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1,420 results on '"Universität Bern [Bern]"'

1. The solar WIND and suprathermal ion composition investigation on the WIND spacecraft

Author: Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI, USA, Department of Physics, University of Maryland, College Park, MD, USA, Physikalisches Institut, Universität Bern, Bern, Switzerland, Institut für Datenverarbeitungsanlagen, Technische Universität Braunschweig, Braunschweig, Germany, High Altitude Observatory (NCAR), Boulder, CO, USA, National Aeronautics and Space Administration/Goddard Space Flight Center, Greenbelt, MD, USA, Department of Physics, University of Maryland, College Park, MD, USA; Physikalisches Institut, Universität Bern, Bern, Switzerland, Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany, Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany, Ann Arbor, Bochsler, P., Balsiger, H., Gloeckler, George, Bürgi, A., Fisk, Len A., Galvin, A.B., Geiss, Johannes, Gliem, F., Hamilton, D.C., Holzer, T.E., Hovestadt, D., Ipavich, F.M., Kirsch, E., Lundgren, R.A., Ogilvie, K.W., Sheldon, R.B., Wilken, B., Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI, USA, Department of Physics, University of Maryland, College Park, MD, USA, Physikalisches Institut, Universität Bern, Bern, Switzerland, Institut für Datenverarbeitungsanlagen, Technische Universität Braunschweig, Braunschweig, Germany, High Altitude Observatory (NCAR), Boulder, CO, USA, National Aeronautics and Space Administration/Goddard Space Flight Center, Greenbelt, MD, USA, Department of Physics, University of Maryland, College Park, MD, USA; Physikalisches Institut, Universität Bern, Bern, Switzerland, Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany, Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany, Ann Arbor, Bochsler, P., Balsiger, H., Gloeckler, George, Bürgi, A., Fisk, Len A., Galvin, A.B., Geiss, Johannes, Gliem, F., Hamilton, D.C., Holzer, T.E., Hovestadt, D., Ipavich, F.M., Kirsch, E., Lundgren, R.A., Ogilvie, K.W., Sheldon, R.B., and Wilken, B.
Abstract: The Solar Wind and Suprathermal Ion Composition Experiment (SMS) on WIND is designed to determine uniquely the elemental, isotopic, and ionic-charge composition of the solar wind, the temperatures and mean speeds of all major solar-wind ions, from H through Fe, at solar wind speeds ranging from 175 kms −1 (protons) to 1280 kms −1 (Fe +8 ), and the composition, charge states as well as the 3-dimensional distribution functions of suprathermal ions, including interstellar pick-up He + , of energies up to 230 keV/e. The experiment consists of three instruments with a common Data Processing Unit. Each of the three instruments uses electrostatic analysis followed by a time-of-flight and, as required, an energy measurement. The observations made by SMS will make valuable contributions to the ISTP objectives by providing information regarding the composition and energy distribution of matter entering the magnetosphere. In addition SMS results will have an impact on many areas of solar and heliospheric physics, in particular providing important and unique information on: (i) conditions and processes in the region of the corona where the solar wind is accelerated; (ii) the location of the source regions of the solar wind in the corona; (iii) coronal heating processes; (iv) the extent and causes of variations in the composition of the solar atmosphere; (v) plasma processes in the solar wind; (vi) the acceleration of particles in the solar wind; and (vii) the physics of the pick-up process of interstellar He as well as lunar particles in the solar wind, and the isotopic composition of interstellar helium.
Published: 2006

2. The Solar Origin of Corotating Interaction Regions and Their Formation in the Inner Heliosphere

Author: Dept. of Atmosph., Oceanic, and Space Sciences, University of Michigan, Ann Arbor, Mich., USA, Dept. of Physics and IPST, University of Maryland, College Park, Maryland, USA; Dept. of Atmosph., Oceanic, and Space Sciences, University of Michigan, Ann Arbor, Mich., USA, Science Applications International Corporation, San Diego, California, USA, International Space Science Institute, Bern, Switzerland, Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge, United Kingdom, The Blackett Laboratory, Imperial College, London, United Kingdom, Extraterrestrische Physik, Universität Kiel, Kiel, Germany, Center for Space Physics, Boston University, Boston, Massachusetts, USA, Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany, Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany, Astrophysikalisches Institut, Potsdam, Germany, NASA/Goddard Space Flight Center, Greenbelt, Maryland, USA; Dept. of Physics and IPST, University of Maryland, College Park, Maryland, USA, Physikalisches Institut der Universität Bern, Bern, Switzerland, E.O. Hulburt Center for Space Research, Naval Research Laboratory, Washington, DC, USA, Ann Arbor, Crooker, N.U., Balogh, A., Bothmer, V., Forsyth, R.J., Gloeckler, George, Hewish, A., Hilchenbach, M., Kallenbach, R., Klecker, B., Linker, J.A., Lucek, E., Mann, G., Marsch, E., Posner, A., Richardson, I.G., Schmidt, J.M., Scholer, M., Wang, Y.-M., Wimmer-Schweingruber, R.F., Aellig, M.R., Bochsler, P., Hefti, S., Mikić, Z., Dept. of Atmosph., Oceanic, and Space Sciences, University of Michigan, Ann Arbor, Mich., USA, Dept. of Physics and IPST, University of Maryland, College Park, Maryland, USA; Dept. of Atmosph., Oceanic, and Space Sciences, University of Michigan, Ann Arbor, Mich., USA, Science Applications International Corporation, San Diego, California, USA, International Space Science Institute, Bern, Switzerland, Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge, United Kingdom, The Blackett Laboratory, Imperial College, London, United Kingdom, Extraterrestrische Physik, Universität Kiel, Kiel, Germany, Center for Space Physics, Boston University, Boston, Massachusetts, USA, Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany, Max-Planck-Institut für Extraterrestrische Physik, Garching, Germany, Astrophysikalisches Institut, Potsdam, Germany, NASA/Goddard Space Flight Center, Greenbelt, Maryland, USA; Dept. of Physics and IPST, University of Maryland, College Park, Maryland, USA, Physikalisches Institut der Universität Bern, Bern, Switzerland, E.O. Hulburt Center for Space Research, Naval Research Laboratory, Washington, DC, USA, Ann Arbor, Crooker, N.U., Balogh, A., Bothmer, V., Forsyth, R.J., Gloeckler, George, Hewish, A., Hilchenbach, M., Kallenbach, R., Klecker, B., Linker, J.A., Lucek, E., Mann, G., Marsch, E., Posner, A., Richardson, I.G., Schmidt, J.M., Scholer, M., Wang, Y.-M., Wimmer-Schweingruber, R.F., Aellig, M.R., Bochsler, P., Hefti, S., and Mikić, Z.
Abstract: Corotating Interaction Regions (CIRs) form as a consequence of the compression of the solar wind at the interface between fast speed streams and slow streams. Dynamic interaction of solar wind streams is a general feature of the heliospheric medium; when the sources of the solar wind streams are relatively stable, the interaction regions form a pattern which corotates with the Sun. The regions of origin of the high speed solar wind streams have been clearly identified as the coronal holes with their open magnetic field structures. The origin of the slow speed solar wind is less clear; slow streams may well originate from a range of coronal configurations adjacent to, or above magnetically closed structures. This article addresses the coronal origin of the stable pattern of solar wind streams which leads to the formation of CIRs. In particular, coronal models based on photospheric measurements are reviewed; we also examine the observations of kinematic and compositional solar wind features at 1 AU, their appearance in the stream interfaces (SIs) of CIRs, and their relationship to the structure of the solar surface and the inner corona; finally we summarise the Helios observations in the inner heliosphere of CIRs and their precursors to give a link between the optical observations on their solar origin and the in-situ plasma observations at 1 AU after their formation. The most important question that remains to be answered concerning the solar origin of CIRs is related to the origin and morphology of the slow solar wind.
Published: 2006

3. Reflection, emission, and polarization properties of surfaces made of hyperfine grains, and implications for the nature of primitive small bodies

Author: Sultana, Robin, Poch, Olivier, Beck, Pierre, Schmitt, B., Quirico, E., Spadaccia, Stefano, Patty, Lucas, Pommerol, Antoine, Maturilli, Alessandro, Helbert, Jörn, Alemanno, Giulia, Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, National Centre of Competence in Research PlanetS (NCCR PlanetS), Physikalisches Institut [Bern], Universität Bern [Bern] (UNIBE)-Universität Bern [Bern] (UNIBE)-Swiss National Science Foundation (SNSF), DLR Institut für Planetenforschung, Deutsches Zentrum für Luft- und Raumfahrt [Berlin] (DLR), European Project: ERC-CoG2017-771691,SOLARYS, and European Project: 654208,Europlanet-2020 RI
Subjects: Earth and Planetary Astrophysics (astro-ph.EP), asteroids, spectroscopy, Space and Planetary Science, [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), small bodies, Astrophysics - Earth and Planetary Astrophysics
Abstract: There are various indications that the most primitive small bodies (P, D-type asteroids, comets) have surfaces made of intimate mixtures of opaque minerals and other components (silicates, carbonaceous compounds, etc.) in the form of sub-micrometre-sized grains, smaller than the wavelength at which they are observed, so-called hyperfine grains. Here, we investigate how the Vis-NIR-MIR spectral and V-band polarimetric properties of surfaces made of hyperfine grains are influenced by the relative abundance of such hyperfine materials, having strongly different optical indexes. Mixtures of grains of olivine and iron sulfide (or anthracite), as analogues of silicates and opaque minerals present on small bodies, were prepared at different proportions. The measurements reveal that these mixtures of hyperfine grains have spectral and polarimetric Vis-NIR properties varying in strongly nonlinear ways. When present at even a few percent, opaque components dominate the Vis-NIR spectral and polarimetric properties, and mask the silicate bands at these wavelengths. The Vis-NIR spectral slope ranges from red (positive slope), for pure opaque material, to blue (negative slope) as the proportion of silicates increases, which is reminiscent of the range of spectral slopes observed on P, D, X, C- and B-types asteroids. The spectra of the darkest mixtures in the Vis-NIR exhibit the absorption bands of Si-O in olivine around 10 m in the MIR, which is observed in emission for several small bodies. This work shows that both the contrasted optical indexes of the components, and the dispersion or aggregation (depending on their relative proportions) of their hyperfine grains, induce different light scattering regimes in the Vis-NIR and MIR, as observed for primitive small bodies. The optical separation of hyperfine grains seems to be a major parameter controlling the optical properties of these objects., accepted in Icarus
Published: 2023

4. Out-of-phase Late Pleistocene glacial maxima in the Western Alps reflect past changes in North Atlantic atmospheric circulation

Author: Christian Crouzet, Pierre G. Valla, Jean-François Buoncristiani, Frank Preusser, Natacha Gribenski, Thibault Roattino, Institute of Geological Sciences [Bern], University of Bern, Institut des Sciences de la Terre (ISTerre), Institut national des sciences de l'Univers (INSU - CNRS)-Institut de recherche pour le développement [IRD] : UR219-Université Grenoble Alpes (UGA)-Université Gustave Eiffel-Centre National de la Recherche Scientifique (CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry]), Institute for Geology [Freiberg] ( Institut für Geologie [Freiberg]), Technishe Universität Bergakademie Freiberg (TU Bergakademie Freiberg), Biogéosciences [UMR 6282] [Dijon] (BGS), Centre National de la Recherche Scientifique (CNRS)-Université de Bourgogne (UB)-AgroSup Dijon - Institut National Supérieur des Sciences Agronomiques, de l'Alimentation et de l'Environnement, Work supported by the Swiss National Science Foundation (grant PP00P2_170559), the Institut National des Sciences de l'Univers, and the Universite Savoie Mont Blanc., Institut für Geologie [Bern], Universität Bern [Bern], Institute of Earth and Environmental Science, University of Freiburg, Université de Bourgogne (UB)-AgroSup Dijon - Institut National Supérieur des Sciences Agronomiques, de l'Alimentation et de l'Environnement-Centre National de la Recherche Scientifique (CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Institut de recherche pour le développement [IRD] : UR219-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Gustave Eiffel-Université Grenoble Alpes (UGA), Universität Bern [Bern] (UNIBE), Biogéosciences [UMR 6282] (BGS), and Université de Bourgogne (UB)-Centre National de la Recherche Scientifique (CNRS)
Subjects: Marine isotope stage, 010506 paleontology, geography, geography.geographical_feature_category, 010504 meteorology & atmospheric sciences, Pleistocene, Thermoluminescence dating, Northern Hemisphere, Geology, Glacier, Last Glacial Maximum, 01 natural sciences, Paleontology, 13. Climate action, [SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/Stratigraphy, [SDE]Environmental Sciences, [SDU.STU.GL]Sciences of the Universe [physics]/Earth Sciences/Glaciology, Glacial period, Foreland basin, 0105 earth and related environmental sciences
Abstract: Paleoglacier reconstructions in the northern and southern forelands of the European Alps indicate a synchronous Late Pleistocene glacial maximum during Marine Isotope Stage (MIS) 2, in phase with global ice volume records. However, strong controversy remains for the western foreland, where scarce and indirect dating as well as modeling studies suggest glacial maxima out of phase with the rest of the Alps. New luminescence dating brings the first direct Late Pleistocene glacial chronology for the western Alpine foreland and reveals two major glacier advances of similar maximum extent, at ca. 75–60 and ca. 40–30 ka, coinciding with MIS 4 and late MIS 3. We propose that asynchrony in glacial maxima between the western and the northern and southern Alpine forelands results from a progressive spatial reorganization of the atmospheric circulation over the North Atlantic in response to Northern Hemisphere ice-sheet fluctuations. While such a feedback mechanism has emerged from general circulation models, our Late Pleistocene paleoglacial reconstruction permits tracking of the spatiotemporal evolution of moisture advection patterns over Western Europe.
Published: 2021

5. Evaluation of global terrestrial evapotranspiration using state-of-the-art approaches in remote sensing, machine learning and land surface modeling

Author: Danica Lombardozzi, Hanqin Tian, Sebastian Lienert, Atul K. Jain, Etsushi Kato, Steven W. Running, Naiqing Pan, Julia E. M. S. Nabel, Pierre Friedlingstein, Catherine Ottlé, Hao Shi, Benjamin Poulter, Stephen Sitch, Sönke Zaehle, Vivek K. Arora, Vanessa Haverd, Shufen Pan, Auburn University (AU), College of Engineering, Mathematics and Physical Sciences [Exeter] (EMPS), University of Exeter, College of Life and Environmental Sciences [Exeter], Canadian Centre for Climate Modelling and Analysis (CCCma), Environment and Climate Change Canada, CSIRO Marine and Atmospheric Research [Aspendale], Commonwealth Scientific and Industrial Research Organisation [Canberra] (CSIRO), Department of Atmospheric Sciences [Urbana], University of Illinois at Urbana-Champaign [Urbana], University of Illinois System-University of Illinois System, Tokyo Institute of Technology [Tokyo] (TITECH), Climate and Environmental Physics [Bern] (CEP), Physikalisches Institut [Bern], Universität Bern [Bern]-Universität Bern [Bern], National Center for Atmospheric Research [Boulder] (NCAR), Max Planck Institute for Meteorology (MPI-M), Max-Planck-Gesellschaft, Laboratoire des Sciences du Climat et de l'Environnement [Gif-sur-Yvette] (LSCE), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ), Modélisation des Surfaces et Interfaces Continentales (MOSAIC), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ), NASA Goddard Space Flight Center (GSFC), Biogeochemical Systems Department [Jena], Max Planck Institute for Biogeochemistry (MPI-BGC), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Montana State University (MSU), Universität Bern [Bern] (UNIBE)-Universität Bern [Bern] (UNIBE), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), and Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)
Subjects: Canopy, 010504 meteorology & atmospheric sciences, 530 Physics, 0208 environmental biotechnology, 02 engineering and technology, lcsh:Technology, 01 natural sciences, lcsh:TD1-1066, Evapotranspiration, lcsh:Environmental technology. Sanitary engineering, [SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces, environment, lcsh:Environmental sciences, 0105 earth and related environmental sciences, General Environmental Science, lcsh:GE1-350, [SDU.OCEAN]Sciences of the Universe [physics]/Ocean, Atmosphere, Physical model, lcsh:T, Water stress, lcsh:Geography. Anthropology. Recreation, 15. Life on land, Arid, Relative stability, 020801 environmental engineering, lcsh:G, 13. Climate action, Remote sensing (archaeology), Climatology, General Earth and Planetary Sciences, Environmental science, Satellite
Abstract: Evapotranspiration (ET) is a critical component in global water cycle and links terrestrial water, carbon and energy cycles. Accurate estimate of terrestrial ET is important for hydrological, meteorological, and agricultural research and applications, such as quantifying surface energy and water budgets, weather forecasting, and scheduling of irrigation. However, direct measurement of global terrestrial ET is not feasible. Here, we first gave a retrospective introduction to the basic theory and recent developments of state-of-the-art approaches for estimating global terrestrial ET, including remote sensing-based physical models, machine learning algorithms and land surface models (LSMs). Then, we utilized six remote sensing-based models (including four physical models and two machine learning algorithms) and fourteen LSMs to analyze the spatial and temporal variations in global terrestrial ET. The results showed that the mean annual global terrestrial ET ranged from 50.7 × 103 km3 yr−1（454 mm yr−1）to 75.7 × 103 km3 yr−1 (6977 mm yr−1), with the average being 65.5 × 103 km3 yr−1 (588 mm yr−1), during 1982–2011. LSMs had significant uncertainty in the ET magnitude in tropical regions especially the Amazon Basin, while remote sensing-based ET products showed larger inter-model range in arid and semi-arid regions than LSMs. LSMs and remote sensing-based physical models presented much larger inter-annual variability (IAV) of ET than machine learning algorithms in southwestern U.S. and the Southern Hemisphere, particularly in Australia. LSMs suggested stronger control of precipitation on ET IAV than remote sensing-based models. The ensemble remote sensing-based physical models and machine-learning algorithm suggested significant increasing trends in global terrestrial ET at the rate of 0.62 mm yr−2 (p 0.05), even though most of the individual LSMs reproduced the increasing trend. Moreover, all models suggested a positive effect of vegetation greening on ET intensification. Spatially, all methods showed that ET significantly increased in western and southern Africa, western India and northeastern Australia, but decreased severely in southwestern U.S., southern South America and Mongolia. Discrepancies in ET trend mainly appeared in tropical regions like the Amazon Basin. The ensemble means of the three ET categories showed generally good consistency, however, considerable uncertainties still exist in both the temporal and spatial variations in global ET estimates. The uncertainties were induced by multiple factors, including parameterization of land processes, meteorological forcing, lack of in situ measurements, remote sensing acquisition and scaling effects. Improvements in the representation of water stress and canopy dynamics are essentially needed to reduce uncertainty in LSM-simulated ET. Utilization of latest satellite sensors and deep learning methods, theoretical advancements in nonequilibrium thermodynamics, and application of integrated methods that fuse different ET estimates or relevant key biophysical variables will improve the accuracy of remote sensing-based models.
Published: 2020

6. Cometary Dust

Author: Anny-Chantal Levasseur-Regourd, Jessica Agarwal, Hervé Cottin, Cécile Engrand, George Flynn, Marco Fulle, Tamas Gombosi, Yves Langevin, Jérémie Lasue, Thurid Mannel, Sihane Merouane, Olivier Poch, Nicolas Thomas, Andrew Westphal, IMPEC - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Sonnensystemforschung (MPS), Max-Planck-Gesellschaft, Laboratoire Interuniversitaire des Systèmes Atmosphériques (LISA (UMR_7583)), Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), State University of New York at Plattsburgh (SUNY Plattsburgh), State University of New York (SUNY), INAF - Osservatorio Astronomico di Trieste (OAT), Istituto Nazionale di Astrofisica (INAF), Department of Climate and Space Sciences and Engineering (CLaSP), University of Michigan [Ann Arbor], University of Michigan System-University of Michigan System, Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Institute of Physics [Graz], University of Graz, Space Research Institute of Austrian Academy of Sciences (IWF), Austrian Academy of Sciences (OeAW), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Physikalisches Institut [Bern], Universität Bern [Bern], Space Sciences Laboratory [Berkeley] (SSL), University of California [Berkeley], University of California-University of California, PLANETO - LATMOS, Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Karl-Franzens-Universität [Graz, Autriche], Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Karl-Franzens-Universität Graz, Universität Bern [Bern] (UNIBE), University of California [Berkeley] (UC Berkeley), University of California (UC)-University of California (UC), and Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12)-Institut national des sciences de l'Univers (INSU - CNRS)
Subjects: Aggregates, Jupiter-family comets, Astrophysics::Cosmology and Extragalactic Astrophysics, 010502 geochemistry & geophysics, 01 natural sciences, complex mixtures, Nucleus, Article, Organics, 0103 physical sciences, Rosetta, Comets, Astrophysics::Solar and Stellar Astrophysics, Coma, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, 0105 earth and related environmental sciences, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], 520 Astronomy, Astronomy and Astrophysics, Dust, 620 Engineering, Stardust, respiratory tract diseases, 13. Climate action, Space and Planetary Science, Physics::Space Physics, Astrophysics::Earth and Planetary Astrophysics, Trail
Abstract: International audience; This review presents our understanding of cometary dust at the end of 2017. For decades, insight about the dust ejected by nuclei of comets had stemmed from remote observations from Earth or Earth’s orbit, and from flybys, including the samples of dust returned to Earth for laboratory studies by the Stardust return capsule. The long-duration Rosetta mission has recently provided a huge and unique amount of data, obtained using numerous instruments, including innovative dust instruments, over a wide range of distances from the Sun and from the nucleus. The diverse approaches available to study dust in comets, together with the related theoretical and experimental studies, provide evidence of the composition and physical properties of dust particles, e.g., the presence of a large fraction of carbon in macromolecules, and of aggregates on a wide range of scales. The results have opened vivid discussions on the variety of dust-release processes and on the diversity of dust properties in comets, as well as on the formation of cometary dust, and on its presence in the near-Earth interplanetary medium. These discussions stress the significance of future explorations as a way to decipher the formation and evolution of our Solar System.
Published: 2022

7. A strong mitigation scenario maintains climate neutrality of northern peatlands

Author: Qiu, Chunjing, Ciais, Philippe, Zhu, Dan, Guenet, Bertrand, Chang, Jinfeng, Chaudhary, Nitin, Kleinen, Thomas, Li, Xinyu, Müller, Jurek, Xi, Yi, Zhang, Wenxin, Ballantyne, Ashley, Brewer, Simon, Brovkin, Victor, Charman, Dan, Gustafson, Adrian, Gallego-Sala, Angela, Gasser, Thomas, Holden, Joseph, Joos, Fortunat, Kwon, Min Jung, Lauerwald, Ronny, Miller, Paul, Peng, Shushi, Page, Susan, Smith, Benjamin, Stocker, Benjamin, Sannel, A. Britta K., Salmon, Elodie, Schurgers, Guy, Shurpali, Narasinha, Wårlind, David, Westermann, Sebastian, Kwon, Min, Laboratoire des Sciences du Climat et de l'Environnement [Gif-sur-Yvette] (LSCE), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Mathématiques et Informatique Appliquées (MIA Paris-Saclay), AgroParisTech-Université Paris-Saclay-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Sino-French Institute for Earth System Science, College of Urban and Environmental Sciences, Peking University [Beijing], Laboratoire de géologie de l'ENS (LGENS), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Département des Géosciences - ENS Paris, École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Ecologie fonctionnelle et écotoxicologie des agroécosystèmes (ECOSYS), European Research Council, ERC: SyG-2013-610028 IMBALANCE-P, Agence Nationale de la Recherche, ANR, This work was supported by the European Research Council Synergy grant (SyG-2013-610028 IMBALANCE-P) and the French State Aid managed by the ANR under the ?Investissements d'avenir? programme (ANR-16-CONV-0003_Cland). ORCHIDEE-PEAT performed simulations using HPC resources from GENCI-TGCC (2020-A0070106328). A.V.G.-S. was funded by the Natural Environment Research Council (NERC standard grant no. NE/I012915/1 and no. NE/S001166/1). W.Z. acknowledges funding from the Swedish Research Council FORMAS 2016-01201 and Swedish National Space Agency 209/19. N.C. acknowledges funding by the Nunataryuk (EU grant agreement no. 773421) and the Swedish Research Council FORMAS (contract no. 2019-01151). LPJ-GUESS_dyn simulations were performed on the supercomputing facilities at the University of Oslo, Norway, and on the Aurora and Tetralith resources of the Swedish National Infrastructure for Computing (SNIC) at the Lund University Centre for Scientific and Technical Computing (Lunarc), project no. 2021/2-61 and no. 2021/2-28, and Link?ping University, project no. snic2020/5-563. A.G. P.A.M. W.Z. B.S. D.W. and N.C. acknowledge support from the strategic research areas Modeling the Regional and Global Earth System (MERGE) and Biodiversity and Ecosystem Services in a Changing Climate (BECC) at Lund University. P.A.M. and D.W. received financial support from the H2020 CRESCENDO project (grant agreement no. 641816). LPJ-GUESS simulations were enabled by resources provided by the Swedish National Infrastructure for Computing (SNIC) at LUNARC partially funded by the Swedish Research Council through grant agreement no. 2018-05973. J.M. and F.J. acknowledge financial support by the Swiss National Science Foundation (no. 200020_172476 and no. 200020_200511) and funding from the European Union's Horizon 2020 research and innovation program under grant agreement no. 820989 (project COMFORT) and no. 821003 (project 4C). The work reflects only the authors views, the European Commission and their executive agency are not responsible for any use that may be made of the information the work contains. B.G. received funding from the European Union's Horizon 2020 research and innovation program under grant agreement no. 641816 (CRESCENDO) and no. 821003 (4C project). B.D.S was funded by the Swiss National Science Foundation grant no. PCEFP2_181115. T.K. acknowledges support from the German Federal Ministry for Education and Research (BMBF) through the PalMod programme (grant no. 01LP1507B and no. 01LP1921A). LPJ-MPI experiments were performed at the German Climate Computing Centre (DKRZ), using resources from the Max Planck Institute for Meteorology. N.J.S. acknowledges financial support from Academy of Finland (no. 296887 and no. 334422) and the Finnish Ministry of Agriculture and Forestry (no. VN/28562/2020). J.C. acknowledged support from the Fundamental Research Funds for the Central Universities (no. 2021QNA6005). D.Z. acknowledges funding from the National Natural Science Foundation of China (grant no. 42101090 and no. 41988101). W.Z and G.S. acknowledge support from the Danish National Research Foundation (DNRF100). C.Q. P.C. D.Z. and B.G. designed the research, C.Q. and P.C. drafted the manuscript, J.C. prepared the climate forcing for ORCHIDEE-PEAT and computed estimates of global and Northern Hemisphere CO2 emissions from ISIMIP2b terrestrial biosphere models, C.Q. N.C. T.K. X.Y.L. J.M. Y.X. and W.Z. performed model simulations, A.V.G.-S. and S.C.B. provided estimates for future peat carbon sink from Gallego-Sala et al.15, all authors contributed to the interpretation of the results and draft revision., ANR-16-CONV-0003,CLAND,CLAND : Changement climatique et usage des terres(2016), European Project: 641816,H2020,H2020-SC5-2014-two-stage,CRESCENDO(2015), ICOS-ATC (ICOS-ATC), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Modélisation des Surfaces et Interfaces Continentales (MOSAIC), Key Laboratory of Plant-Soil Interactions - College of Resources and Environmental Sciences (PSI), China Agricultural University (CAU), Department of Geosciences [Oslo], Faculty of Mathematics and Natural Sciences [Oslo], University of Oslo (UiO)-University of Oslo (UiO), Department of Physical Geography and Ecosystem Science [Lund], Lund University [Lund], Max Planck Institute for Meteorology (MPI-M), Max-Planck-Gesellschaft, Climate and Environmental Physics [Bern] (CEP), Physikalisches Institut [Bern], Universität Bern [Bern] (UNIBE)-Universität Bern [Bern] (UNIBE), Oeschger Centre for Climate Change Research (OCCR), University of Bern, Center for Permafrost (CENPERM), Department of Geosciences and Natural Resource Management [Copenhagen] (IGN), Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH)-Faculty of Science [Copenhagen], University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH), Department of Ecosystem and Conservation Sciences, University of Montana, University of Utah, College of Life and Environmental Sciences [Exeter], University of Exeter, International Institute for Applied Systems Analysis [Laxenburg] (IIASA), School of Geography [Leeds], University of Leeds, University of Leicester, Hawkesbury Institute for the Environment [Richmond] (HIE), Western Sydney University, Department of Environmental Systems Science [ETH Zürich] (D-USYS), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Swiss Federal Institute for Forest, Snow and Landscape Research WSL, Department of Physical Geography [Stockholm], Stockholm University, Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), and Natural Resources Institute Finland (LUKE)
Subjects: [SDU.OCEAN]Sciences of the Universe [physics]/Ocean, Atmosphere, 0303 health sciences, 010504 meteorology & atmospheric sciences, 530 Physics, methane, [SDE.MCG]Environmental Sciences/Global Changes, carbon dioxide, carbon-cycle feedback, 15. Life on land, 01 natural sciences, 03 medical and health sciences, long-term climate change, 13. Climate action, [SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology, land surface models, Earth and Planetary Sciences (miscellaneous), peatland, [SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces, environment, 030304 developmental biology, 0105 earth and related environmental sciences, General Environmental Science, permafrost
Abstract: Northern peatlands store 300–600 Pg C, of which approximately half are underlain by permafrost. Climate warming and, in some regions, soil drying from enhanced evaporation are progressively threatening this large carbon stock. Here, we assess future CO2 and CH4 fluxes from northern peatlands using five land surface models that explicitly include representation of peatland processes. Under Representative Concentration Pathways (RCP) 2.6, northern peatlands are projected to remain a net sink of CO2 and climate neutral for the next three centuries. A shift to a net CO2 source and a substantial increase in CH4 emissions are projected under RCP8.5, which could exacerbate global warming by 0.21°C (range, 0.09–0.49°C) by the year 2300. The true warming impact of peatlands might be higher owing to processes not simulated by the models and direct anthropogenic disturbance. Our study highlights the importance of understanding how future warming might trigger high carbon losses from northern peatlands.
Published: 2022

8. Spatial variations in Leishmaniasis: A biogeographic approach to mapping the distribution of Leishmania species

Author: Marine Ginouves, Pierre Couppié, Rodolphe E. Gozlan, Ghislaine Prévot, Marine Combe, Mathieu Nacher, Soushieta Jagadesh, Stéphane Simon, Institute of Social and Preventive Medicine [Bern] (ISPM), Universität Bern [Bern] (UNIBE), Institut des Sciences de l'Evolution de Montpellier (UMR ISEM), Centre de Coopération Internationale en Recherche Agronomique pour le Développement (Cirad)-École Pratique des Hautes Études (EPHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Montpellier (UM)-Institut de recherche pour le développement [IRD] : UR226-Centre National de la Recherche Scientifique (CNRS), Biome Tropical et Immuno-Pathophysiologie = Tropical Biome and ImmunoPhysiopathology [Lille] (TBIP), Centre d’Infection et d’Immunité de Lille - INSERM U 1019 - UMR 9017 - UMR 8204 (CIIL), Institut Pasteur de Lille, Réseau International des Instituts Pasteur (RIIP)-Réseau International des Instituts Pasteur (RIIP)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université de Lille-Centre Hospitalier Régional Universitaire [Lille] (CHRU Lille)-Centre National de la Recherche Scientifique (CNRS)-Institut Pasteur de Lille, Réseau International des Instituts Pasteur (RIIP)-Réseau International des Instituts Pasteur (RIIP)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université de Lille-Centre Hospitalier Régional Universitaire [Lille] (CHRU Lille)-Centre National de la Recherche Scientifique (CNRS)-Université de Guyane (UG), Centre Hospitalier Andrée Rosemon [Cayenne, Guyane Française], Centre d'Investigation Clinique Antilles-Guyane (CIC - Antilles Guyane), Université des Antilles et de la Guyane (UAG)-Institut National de la Santé et de la Recherche Médicale (INSERM)-CHU Pointe-à-Pitre/Abymes [Guadeloupe] -CHU de Fort de France-Centre Hospitalier Andrée Rosemon [Cayenne, Guyane Française], Universität Bern [Bern], École pratique des hautes études (EPHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Montpellier (UM)-Centre de Coopération Internationale en Recherche Agronomique pour le Développement (Cirad)-Centre National de la Recherche Scientifique (CNRS)-Institut de recherche pour le développement [IRD] : UR226, Centre National de la Recherche Scientifique (CNRS)-Centre Hospitalier Régional Universitaire [Lille] (CHRU Lille)-Université de Lille-Institut National de la Santé et de la Recherche Médicale (INSERM)-Institut Pasteur de Lille, Réseau International des Instituts Pasteur (RIIP)-Réseau International des Instituts Pasteur (RIIP)-Centre National de la Recherche Scientifique (CNRS)-Centre Hospitalier Régional Universitaire [Lille] (CHRU Lille)-Université de Lille-Institut National de la Santé et de la Recherche Médicale (INSERM)-Institut Pasteur de Lille, Réseau International des Instituts Pasteur (RIIP)-Réseau International des Instituts Pasteur (RIIP)-Université de Guyane (UG), CHU de Fort de France-Centre Hospitalier Andrée Rosemon [Cayenne, Guyane Française]-CHU Pointe-à-Pitre/Abymes [Guadeloupe] -Institut National de la Santé et de la Recherche Médicale (INSERM)-Université des Antilles et de la Guyane (UAG), Centre de Coopération Internationale en Recherche Agronomique pour le Développement (Cirad)-École pratique des hautes études (EPHE), and Matillon, Mirlène
Subjects: Medicine (General), [SDV]Life Sciences [q-bio], 030231 tropical medicine, Stacked species distribution modelling, Spatial distribution, 03 medical and health sciences, Zoonosis, 0302 clinical medicine, R5-920, Cutaneous leishmaniasis, parasitic diseases, medicine, Deforestation, Endemism, 030304 developmental biology, One health, 0303 health sciences, biology, Ecology, Public Health, Environmental and Occupational Health, Leishmaniasis, medicine.disease, Leishmania, biology.organism_classification, Environmental niche modelling, [SDV] Life Sciences [q-bio], Infectious Diseases, Biogeography, 13. Climate action, Vector (epidemiology), Spatial ecology, Research Paper
Abstract: Cutaneous Leishmaniasis (CL) is the most prevalent form of Leishmaniasis and is widely endemic in the Americas. Several species of Leishmania are responsible for CL, a severely neglected tropical disease and the treatment of CL vary according to the different species of Leishmania. We proposed to map the distribution of the Leishmania species reported in French Guiana (FG) using a biogeographic approach based on environmental predictors. We also measured species endemism i.e., the uniqueness of species to a defined geographic location. Our results show that the distribution patterns varied between Leishmania spp. and were spatially dependent on climatic covariates. The species distribution modelling of the eco-epidemiological spatial patterns of Leishmania spp. is the first to measure endemism based on bioclimatic factors in FG. The study also emphasizes the impact of tree cover loss and climate on the increasing distribution of L. (Viannia) braziliensis in the most anthropized regions. Detection of high-risk regions for the different between Leishmania spp. is essential for monitoring and active surveillance of the vector. As climate plays a major role in the spatial distribution of the vector and reservoir and the survival of the pathogen, climatic covariates should be included in the analysis and mapping of vector-borne diseases. This study underscores the significance of local land management and the urgency of considering the impact of climate change in the development of vector-borne disease management strategies at the global scale., Graphical abstract Unlabelled Image
Published: 2021

9. Narrow belt of debris around the Sco-Cen star HD 141011

Author: Virginie Faramaz, Christophe Pinte, Beth Biller, Raphael Galicher, Silvano Desidera, R. Gratton, Mickael Bonnefoy, Mariangela Bonavita, C. Lazzoni, Anthony Boccaletti, Johan Olofsson, Elisabeth Matthews, Philippe Delorme, J. L. Beuzit, C. Mordasini, Julien Milli, Gael Chauvin, Jean-Charles Augereau, A-M. Lagrange, David Mouillet, François Ménard, A. Chomez, Arthur Vigan, Dino Mesa, Sasha Hinkley, Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA), INAF - Osservatorio Astronomico di Padova (OAPD), Istituto Nazionale di Astrofisica (INAF), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Laboratoire de l'intégration, du matériau au système (IMS), Centre National de la Recherche Scientifique (CNRS)-Institut Polytechnique de Bordeaux-Université Sciences et Technologies - Bordeaux 1, University of Edinburgh, Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), University of Arizona, University of Exeter, Observatoire Astronomique de l'Université de Genève (ObsGE), Université de Genève (UNIGE), Massachusetts Institute of Technology (MIT), Universität Bern [Bern], Universidad de Valparaiso [Chile], ANR-14-CE33-0018,GIPSE,Exploration des planetes géantes extrasolaires(2014), ANR-20-CE31-0012,FRAME,Détection et Caractérisation des Exoplanètes en Formation(2020), European Project: 885593,COBREX, European Project: 776403,EXOPLANET, Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut Polytechnique de Bordeaux-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université de Genève = University of Geneva (UNIGE), Universität Bern [Bern] (UNIBE), Université Grenoble Alpes (UGA), National Hospital for Neurology and Neurosurgery [London, UK], and Université Sciences et Technologies - Bordeaux 1-Institut Polytechnique de Bordeaux-Centre National de la Recherche Scientifique (CNRS)
Subjects: 530 Physics, FOS: Physical sciences, Context (language use), Astrophysics, 01 natural sciences, planetary systems -stars, 0103 physical sciences, individual, 010303 astronomy & astrophysics, planetary systems, Solar and Stellar Astrophysics (astro-ph.SR), Physics, Earth and Planetary Astrophysics (astro-ph.EP), 010308 nuclear & particles physics, 520 Astronomy, James Webb Space Telescope, stars: individual: HD 141011 (HIP 77432), techniques: high angular resolution, Astronomy and Astrophysics, Planetary system, Position angle, stars: imaging, Radial velocity, Stars, Fomalhaut, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, HD 141011 (HIP 77432), Halo, techniques, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], high contrast imaging-stars, Astrophysics - Earth and Planetary Astrophysics
Abstract: We initiated a deep-imaging survey of Scorpius-Centaurus A-F stars with predicted warm inner and cold outer belts of debris reminiscent of the architecture of emblematic systems such as HR 8799. We present resolved SPHERE images of a narrow ring of debris around the F5-type star HD 141011 that was observed as part of our survey in 2015, 2016, and 2019. The ring extends up to ~1.1" (~141 au) from the star in the IRDIS and IFS data obtained in 2016 and 2019. The disk is not detected in the 2015 data which are of poorer quality. The disks is best reproduced by models of a noneccentric ring centered on the star with an inclination of $69.1\pm0.9^{\circ}$, a position angle of $-24.6 \pm 1.7^{\circ}$, and a semimajor axis of $127.5\pm3.8$ au. The combination of radial velocity and imaging data excludes brown-dwarf (M>13.6 MJup) companions coplanar with the disk from 0.1 to 0.9 au and from 20 au up to 500 au (90% probability). HD 141011 adds to the growing list of debris disks that are resolved in Sco-Cen. It is one of the faintest disks that are resolved from the ground and has a radial extent and fractional width ($\sim$12.5%) reminiscent of Fomalhaut. Its moderate inclination and large semimajor axis make it a good target for the James Webb Space Telescope and should allow a deeper search for putative companions shaping the dust distribution., 13 pages, 10 figures. Paper II of our Sco-Cen imaging survey. Accepted in A&A
Published: 2021

10. Detecting life outside our solar system with a large high-contrast-imaging mission

Author: Ignasi Ribas, Th. Henning, P. Baudoz, M. Kasper, Pieter J. de Visser, Simon Albrecht, A.-M. Lagrange, Kevin Heng, Enric Palle, Didier Queloz, Nathan J. Mayne, Isabella Pagano, B.-O. Demory, Michiel Min, Olivier Guyon, R. van Boekel, Manuel López-Puertas, Ignas Snellen, Matthew A. Kenworthy, Guillem Anglada-Escudé, Daphne Stam, Julien Milli, Nikku Madhusudhan, Timothy M. Lenton, Garreth Ruane, John Lee Grenfell, Willy Benz, Christopher C. Stark, Valentina D'Orazi, Silvano Desidera, Mamadou N'Diaye, David Mouillet, E. J. W. de Mooij, Mark Claire, Christoph U. Keller, R. G. Gratton, Franck Selsis, A. L. Maire, Elsa Huby, Giampaolo Piotto, Alessandro Sozzetti, Jean-Luc Beuzit, Michaël Gillon, Anthony Boccaletti, Jayne Birkby, Matteo Brogi, Yamila Miguel, Arthur Vigan, Frans Snik, Beth Biller, B. S. Gaudi, Giuseppina Micela, Christiane Helling, Isabelle Baraffe, Oliver Krause, J. de Boer, Laura Kreidberg, Heike Rauer, Jean-Michel Desert, Markus Janson, Riccardo Claudi, Victoria S. Meadows, Ralf Launhardt, L. Carone, Lars A. Buchhave, Sasha Hinkley, Bertrand Mennesson, Leiden Observatory [Leiden], Universiteit Leiden, Sterrewacht Leiden, Centre de Recherche Astrophysique de Lyon (CRAL), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, Université Paris sciences et lettres (PSL), Physikalisches Institut [Bern], Universität Bern [Bern] (UNIBE), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, Institute for Astronomy [Edinburgh] (IfA), University of Edinburgh, Universiteit Leiden [Leiden], École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Universität Bern [Bern], Institut de Planétologie et d'Astrophysique de Grenoble (IPAG ), Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Joseph Louis LAGRANGE (LAGRANGE), Université Côte d'Azur (UCA)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS), Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Low Energy Astrophysics (API, FNWI), University of St Andrews. School of Earth & Environmental Sciences, University of St Andrews. St Andrews Centre for Exoplanet Science, University of St Andrews. St Andrews Isotope Geochemistry, University of St Andrews. School of Physics and Astronomy, European Commission, European Research Council, Science and Technology Facilities Council (UK), Agencia Estatal de Investigación (España), Ministerio de Ciencia, Innovación y Universidades (España), Generalitat de Catalunya, Agenzia Spaziale Italiana, Istituto Nazionale di Astrofisica, Netherlands Organization for Scientific Research, Knut and Alice Wallenberg Foundation, Snellen, IAG [0000-0003-1624-3667], and Apollo - University of Cambridge Repository
Subjects: Solar System, life, Computer science, 01 natural sciences, 010309 optics, White paper, Spitzer Space Telescope, Planet, 0103 physical sciences, Agency (sociology), QB Astronomy, 010303 astronomy & astrophysics, QC, QB, [PHYS]Physics [physics], 520 Astronomy, imaging, Astronomy and Astrophysics, High contrast imaging, 3rd-DAS, 620 Engineering, QC Physics, mission, Space and Planetary Science, 5101 Astronomical Sciences, [SDU]Sciences of the Universe [physics], Extraterrestrial life, Systems engineering, Circumstellar habitable zone, 51 Physical Sciences
Abstract: Snellen, I.A.G. et al., In this White Paper, which was submitted in response to the European Space Agency (ESA) Voyage 2050 Call, we recommend the ESA plays a proactive role in developing a global collaborative effort to construct a large high-contrast imaging space telescope, e.g. as currently under study by NASA. Such a mission will be needed to characterize a sizable sample of temperate Earth-like planets in the habitable zones of nearby Sun-like stars and to search for extraterrestrial biological activity. We provide an overview of relevant European expertise, and advocate ESA to start a technology development program towards detecting life outside the Solar System., I.S. acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program under grant agreement No 694513. A.L.M. acknowledges the financial support of the F.R.S.-FNRS through a postdoctoral researcher grant. MB acknowledges support from the UK Science and Technology Facilities Council (STFC) research grant ST/S000631/1. I.R. acknowledges support from the Spanish Ministry of Science and Innovation and the European Regional Development Fund through grant PGC2018-098153-B-C33, as well as the support of the Generalitat de Catalunya/CERCA programme. E.P. acknowledges support from the Spanish Ministry of Science through grant PGC2018-098153-B-C31. J.M.D. acknowledges funding from the European Research Council (ERC) under the European Unions Horizon 2020 research and innovation programme (grant agreement no. 679633; Exo-Atmos) Part of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. We acknowledge financial support from the ASI-INAF agreement n.2018-16-HH.0 We acknowledge financial support from Spanish MCIU SEV-2017-0709 and PID2019-110689RB-I00 awards. We acknowledge financial support from the ASI-INAF agreement n.2018-16-HH.0 AV acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 757561). KH acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 771620). NJM acknowledges funding from the Leverhulme Trust, and a Science and Technology Facilities Council Consolidated Grant (ST/R000395/1). PdV acknowledges funding from the Netherlands Organisation for Scientific Research NWO (Veni Grant No. 639.041.750). IP acknowledges financial support from the ASI-INAF agreements 2019-29-HH.06-HH.0 and 2015-019-R.1-2018. FS acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement no. 678194; FALCONER). MJ acknowledges support from the Knut and Alice Wallenberg foundation (KAW). JLB acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program under grant agreement No 805445. T.H. acknowledges support from the European Research Council under the Horizon 2020 Framework Program via the ERC Advanced Grant Origins 83 24 28. JLG acknowledges ISSI Team 464 for useful discussion.
Published: 2021

11. Martian meteorites reflectance and implications for rover missions

Author: Pierre Beck, C. Quantin-Nataf, Violaine Sautter, M. Martinot, Lu Pan, Erwin Dehouck, Antoine Pommerol, Romain Cerubini, Lucia Mandon, Zurine Yoldi, Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement (LGL-TPE), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Université Jean Monnet - Saint-Étienne (UJM)-Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, Universität Bern [Bern] (UNIBE), Physikalisches Institut [Bern], Institut de minéralogie, de physique des matériaux et de cosmochimie (IMPMC), Muséum national d'Histoire naturelle (MNHN)-Institut de recherche pour le développement [IRD] : UR206-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement [Lyon] (LGL-TPE), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-École normale supérieure - Lyon (ENS Lyon), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA), and Universität Bern [Bern]
Subjects: spectroscopy, 010504 meteorology & atmospheric sciences, Imaging spectrometer, Mineralogy, FOS: Physical sciences, Mars, 01 natural sciences, Spectral line, meteorites, Physics - Geophysics, 0103 physical sciences, surface, 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), 0105 earth and related environmental sciences, Martian, Earth and Planetary Astrophysics (astro-ph.EP), [PHYS]Physics [physics], Spectrometer, 520 Astronomy, Hyperspectral imaging, Astronomy and Astrophysics, Mars Exploration Program, 620 Engineering, Geophysics (physics.geo-ph), Imaging spectroscopy, Meteorite, Space and Planetary Science, Astrophysics - Instrumentation and Methods for Astrophysics, Geology, Astrophysics - Earth and Planetary Astrophysics
Abstract: International audience; During this decade, two rovers will characterize in situ the mineralogy of rocks on Mars, using for the first time near-infrared reflectance spectrometers: SuperCam onboard the Mars 2020 rover and MicrOmega onboard the ExoMars rover, although this technique is predominantly used in orbit for mineralogical investigations. Until successful completion of sample-return missions from Mars, Martian meteorites are currently the only samples of the red planet available for study in terrestrial laboratories and comparison with in situ data. However, the current spectral database available for these samples does not represent their diversity and consists primarily of spectra acquired on finely crushed samples, albeit grain size is known to greatly affect spectral features. Here, we measured the reflected light of a broad Martian meteorite suite as a means to catalogue and characterize their spectra between 0.4 and 3 μm. These measurements are achieved using a point spectrometer acquiring data comparable to SuperCam, and an imaging spectrometer producing hyperspectral cubes, similarly to MicrOmega. Our results indicate that point spectrometry is sufficient to discriminate the different Martian meteorites families, to identify their primary petrology based on band parameters, and to detect their low content in alteration minerals. However, significant spectral mixing occurs in the point measurements, even at spot sizes down to a few millimeters, and high-resolution imaging spectroscopy is needed to correctly identify the various mineral phases in the meteorites. Additional bidirectional spectral measurements on a consolidated and powdered shergottite confirm their non-Lambertian behavior, with backward and suspected forward scattering peaks. With changing observation geometry, the main absorption strengths show variations up to ~10–15%. The variation of reflectance levels is reduced for the rock surface compared to the powder. All the spectra presented are provided in the supplementary data for further comparison with in situ and orbital measurements.
Published: 2021

12. Olive groves around the lake. A ten-thousand-year history of a Cretan landscape (Greece) reveals the dominant role of humans in making this Mediterranean ecosystem

Author: Roberto Sulpizio, Isabelle Jouffroy-Bapicot, Maxime Debret, Sophie Field, Kevin Walsh, Neil Roberts, Boris Vannière, Pierre Sabatier, Giovanni Zanchetta, Tiziana Pedrotta, Willy Tinner, Laboratoire Chrono-environnement - CNRS - UBFC (UMR 6249) (LCE), Centre National de la Recherche Scientifique (CNRS)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC), Maison des Sciences de l'Homme et de l'Environnement Claude Nicolas Ledoux (UAR 3124) (MSHE), Oeschger Centre for Climate Change Research (OCCR), University of Bern, Morphodynamique Continentale et Côtière (M2C), Université de Caen Normandie (UNICAEN), Normandie Université (NU)-Normandie Université (NU)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rouen Normandie (UNIROUEN), Normandie Université (NU)-Centre National de la Recherche Scientifique (CNRS), School of Geography, Earth and Environmental Sciences [Plymouth] (SoGEES), Plymouth University, University of Bari Aldo Moro (UNIBA), University of Pisa - Università di Pisa, Environnements, Dynamiques et Territoires de la Montagne (EDYTEM), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Institut d'Etudes Avancées [AMU] (IMéRA), Aix Marseille Université (AMU), Universität Bern [Bern], Centre National de la Recherche Scientifique (CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry]), Laboratoire Chrono-environnement (UMR 6249) (LCE), Università degli studi di Bari Aldo Moro = University of Bari Aldo Moro (UNIBA), Environnements, Dynamiques et Territoires de Montagne (EDYTEM), Universität Bern [Bern] (UNIBE), Maison des Sciences de l'Homme et de l'Environnement Claude Nicolas Ledoux (MSHE), Dipartimento di Scienze Delle Terra, University of Pisa, School of Archaeology, University of Oxford, and BioArCh, Department of Archaeology, University of York, York, YO10 5NG, UK
Subjects: 010506 paleontology, Archeology, [SHS.ARCHEO]Humanities and Social Sciences/Archaeology and Prehistory, Biodiversity, Climate change, Woodland, Land cover, Socio-ecosystem, Mediterranean, 010502 geochemistry & geophysics, 01 natural sciences, Anthropisation, Crete, Holocene, Human impacts, Land-use, Olive grove, Paleoecology, 11. Sustainability, 14. Life underwater, ComputingMilieux_MISCELLANEOUS, Ecology, Evolution, Behavior and Systematics, 0105 earth and related environmental sciences, Global and Planetary Change, Land use, Flood myth, Ecology, Geology, Vegetation, 15. Life on land, Geography, 13. Climate action, [SHS.ENVIR]Humanities and Social Sciences/Environmental studies, [SDE]Environmental Sciences
Abstract: (IF 4.45: Q1); International audience; The reconstruction of millennial-scale interactions between ecosystems and societies can provide unique and valuable references for understanding the creation of cultural landscapes and help elucidate their value, weaknesses and legacies. Among the most emblematic forms of Mediterranean land use, olive groves and pastoralism have occupied a prominent place. Therefore, it is vital to know when, how, and with what ecological consequences these practices were established and developed. Located in the southern part of the Aegean Sea, Crete is the largest island of Greece. The island is characterised by a long human history of land use, but our understanding of past environmental changes for the entire Holocene is fragmentary. This paper presents a new investigation of Lake Kournas in Crete, where recent coring provided a 15-m sequence covering ten millennia of land cover and land-use history. The study of this new core involves the analysis of the sediment dynamics, flood deposits, pollen, diatoms, fungal and algal remains, and microcharcoals. Results show that ecosystem development near Lake Kournas was not a linear process. They reveal linkages and feedbacks between vegetation, biodiversity, fire, human impact, erosion, and climate change. A possible human occupation and agro-pastoral activities around the lake may have been detected as early as 9500 cal BP, perhaps in a transitional phase between the Mesolithic and the Neolithic. At 8500 cal BP, climatic conditions may have promoted the expansion of the evergreen oak woodland. However, human impact was probably the most important driver of ecosystem change with the establishment of an agro-system after 8000 years ago. Thereafter, the trajectory of Kournas’ lake and catchment ecosystems from the Mid to Late Holocene follow the rhythm of land-use change. Among the traditional Mediterranean land uses, olive cultivation locally played a major role in the socio-ecosystem interactions, providing economic benefits but also destabilising soils. During the last six millennia, three main phases of olive cultivation occurred during the Final Neolithic-Minoan period, the Hellenistic-Roman-Byzantine (HRB) period and Modern times. Along with the changing land use under the successive political and economic influences rules, the resilience capacities of vegetation permitted it to shift back to higher biodiversity again after decreasing phases. Forest vegetation was always able to recover until the onset of the Venetian period (13th century), when woodlands were dramatically reduced. Only during the past century has forest vegetation slightly recovered, while the flood regime had already been altered during previous centuries. During the past 100 years, biodiversity markedly declined, probably in response to the industrialization of agriculture.
Published: 2021

13. In Situ exploration of the giant planets

Author: Don Banfield, Olivier Mousis, Mark Hofstadter, Leigh N. Fletcher, Sushil K. Atreya, Jean-Pierre Lebreton, Athena Coustenis, Francesca Ferri, Magali Deleuil, Peter Wurz, Kathleen Mandt, Thibault Cavalié, J. Hunter Waite, Thomas R. Spilker, Paul Hartogh, Heike Rauer, Kunio M. Sayanagi, Ethiraj Venkatapathy, Thierry Fouchet, Stas Barabash, Amy Simon, Tristan Guillot, R. Hueso, Jean-Baptiste Renard, Agustín Sánchez-Lavega, Michel Blanc, Richard M. Ambrosi, David H. Atkinson, Pascal Rannou, Georges Durry, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), ASP 2021, Laboratoire d'Astrophysique de Bordeaux [Pessac] (LAB), Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Observatoire de la Côte d'Azur (OCA), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'astrophysique de l'observatoire de Besançon (UMR 6091) (LAOB), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC), Radio and Space Plasma Physics Group [Leicester] (RSPP), University of Leicester, Department of Atmospheric, Oceanic, and Space Sciences [Ann Arbor] (AOSS), University of Michigan [Ann Arbor], University of Michigan System-University of Michigan System, Cornell University [New York], Swedish Institute of Space Physics [Uppsala] (IRF), PSA Peugeot - Citroën (PSA), PSA Peugeot Citroën (PSA), ASP 2019, Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Groupe de spectrométrie moléculaire et atmosphérique (GSMA), Université de Reims Champagne-Ardenne (URCA)-Centre National de la Recherche Scientifique (CNRS), Centro di Ateneo di Studi e Attività Spaziali 'Giuseppe Colombo' (CISAS), Universita degli Studi di Padova, Joseph Louis LAGRANGE (LAGRANGE), Université Côte d'Azur (UCA)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Sonnensystemforschung (MPS), Max-Planck-Gesellschaft, Departamento de Fisica Aplicada [Bilbao], Universidad del Pais Vasco / Euskal Herriko Unibertsitatea [Espagne] (UPV/EHU), Groupe de Recherche sur les Institutions, le Droit de l'Aménagement, de l'Urbanisme et de l'Habitat (GRIDAUH), DLR Institut für Planetenforschung, Deutsches Zentrum für Luft- und Raumfahrt [Berlin] (DLR), Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Space Science Division [San Antonio], Southwest Research Institute [San Antonio] (SwRI), Physikalisches Institut [Bern], Universität Bern [Bern], Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Università degli Studi di Padova = University of Padua (Unipd), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research (MPS), and Universität Bern [Bern] (UNIBE)
Subjects: Exploration of Saturn, Atmospheres, Solar System, 010504 meteorology & atmospheric sciences, Galileo Probe, [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], Formation, FOS: Physical sciences, 01 natural sciences, 7. Clean energy, Astrobiology, Jupiter, Entry probes, Neptune, Planet, Saturn, 0103 physical sciences, Giant planets, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, Earth and Planetary Astrophysics (astro-ph.EP), Uranus, Entry probes · Giant planets · Formation · Composition · Atmospheres, Astronomy and Astrophysics, [SDU]Sciences of the Universe [physics], 13. Climate action, Space and Planetary Science, Physics::Space Physics, Astrophysics::Earth and Planetary Astrophysics, Composition, Astrophysics - Earth and Planetary Astrophysics
Abstract: Remote sensing observations suffer significant limitations when used to study the bulk atmospheric composition of the giant planets of our solar system. This impacts our knowledge of the formation of these planets and the physics of their atmospheres. A remarkable example of the superiority of in situ probe measurements was illustrated by the exploration of Jupiter, where key measurements such as the determination of the noble gases' abundances and the precise measurement of the helium mixing ratio were only made available through in situ measurements by the Galileo probe. Here we describe the main scientific goals to be addressed by the future in situ exploration of Saturn, Uranus, and Neptune, placing the Galileo probe exploration of Jupiter in a broader context. An atmospheric entry probe targeting the 10-bar level would yield insight into two broad themes: i) the formation history of the giant planets and that of the Solar System, and ii) the processes at play in planetary atmospheres. The probe would descend under parachute to measure composition, structure, and dynamics, with data returned to Earth using a Carrier Relay Spacecraft as a relay station. An atmospheric probe could represent a significant ESA contribution to a future NASA New Frontiers or flagship mission to be launched toward Saturn, Uranus, and/or Neptune., 27 pages, 9 figures, White Paper submitted in response to ESA's Call for Voyage 2050 Science Themes. arXiv admin note: substantial text overlap with arXiv:1708.00235
Published: 2021

14. AMBITION – comet nucleus cryogenic sample return

Author: Hervé Cottin, Carsten Güttler, Stavro Ivanoski, Colin Snodgrass, Claudio Codella, Jean-Baptiste Vincent, Kelly E. Miller, Pierre Henri, Maria Drozdovskaya, Alain Herique, Gianrico Filacchione, Kathrin Altwegg, Nicolas Thomas, Martin Bizzarro, Maria Cristina De Sanctis, Rosita Kokotanekova, E. Bianchi, Björn Davidsson, Lydie Bonal, Stefan Ulamec, Cécile Engrand, Cecilia Tubiana, Dominique Bockelée-Morvan, Mathieu Choukroun, Anny Chantal Levasseur-Regourd, Marina Galand, Alessandra Rotundi, Jürgen Blum, M. Schönbächler, Fabrizio Capaccioni, Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS), Istituto Nazionale di Astrofisica (INAF), Physikalisches Institut [Bern], Universität Bern [Bern] (UNIBE), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, Centre for Star and Planet Formation (STARPLAN), Globe Institute, Faculty of Health and Medical Sciences, University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH)-Faculty of Health and Medical Sciences, University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH), Natural History Museum of Denmark, Faculty of Science [Copenhagen], Institut für Geophysik und Extraterrestrische Physik [Braunschweig] (IGEP), Technische Universität Braunschweig = Technical University of Braunschweig [Braunschweig], Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), INAF - Osservatorio Astrofisico di Arcetri (OAA), Laboratoire Interuniversitaire des Systèmes Atmosphériques (LISA (UMR_7583)), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Center for Space and Habitability (CSH), University of Bern, Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Department of Physics [Imperial College London], Imperial College London, Max-Planck-Institut für Sonnensystemforschung (MPS), Max-Planck-Gesellschaft, Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Joseph Louis LAGRANGE (LAGRANGE), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astronomico di Trieste (OAT), European Southern Observatory (ESO), PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Southwest Research Institute [San Antonio] (SwRI), Dipartimento di Scienze e Tecnologie [Napoli] (DIST), Università degli Studi di Napoli 'Parthenope' = University of Naples (PARTHENOPE), Department of Earth Sciences [Swiss Federal Institute of Technology - ETH Zürich] (D-ERDW), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Institute for Astronomy [Edinburgh] (IfA), University of Edinburgh, German Aerospace Center (DLR), DLR Institut für Planetenforschung, Deutsches Zentrum für Luft- und Raumfahrt [Berlin] (DLR), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Universität Bern [Bern], Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA), University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU)-Faculty of Health and Medical Sciences, University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Paris (UP)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National d’Études Spatiales [Paris] (CNES), Université Nice Sophia Antipolis (... - 2019) (UNS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Universita degli studi di Napoli 'Parthenope' [Napoli], Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université Côte d'Azur (UCA)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12)-Centre National de la Recherche Scientifique (CNRS), Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Space and Atmospheric Physics Group [London], Blackett Laboratory, and Imperial College London-Imperial College London
Subjects: Solar System, 010504 meteorology & atmospheric sciences, Comet, Context (language use), 01 natural sciences, Space missions, Space exploration, Astrobiology, Comet nucleus, 0103 physical sciences, Comets, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, Solar system, 520 Astronomy, Giant planet, Astronomy and Astrophysics, 620 Engineering, 13. Climate action, Space and Planetary Science, Asteroid, [SDU]Sciences of the Universe [physics], Formation and evolution of the Solar System, Geology
Abstract: We describe the AMBITION project, a mission to return the first-ever cryogenically-stored sample of a cometary nucleus, that has been proposed for the ESA Science Programme Voyage 2050. Comets are the leftover building blocks of giant planet cores and other planetary bodies, and fingerprints of Solar System’s formation processes. We summarise some of the most important questions still open in cometary science and Solar System formation after the successful Rosetta mission. We show that many of these scientific questions require sample analysis using techniques that are only possible in laboratories on Earth. We summarize measurements, instrumentation and mission scenarios that can address these questions. We emphasize the need for returning a sample collected at depth or, still more challenging, at cryogenic temperatures while preserving the stratigraphy of the comet nucleus surface layers. We provide requirements for the next generation of landers, for cryogenic sample acquisition and storage during the return to Earth. Rendezvous missions to the main belt comets and Centaurs, expanding our knowledge by exploring new classes of comets, are also discussed. The AMBITION project is discussed in the international context of comet and asteroid space exploration.
Published: 2021

15. CHO-Bearing Molecules in Comet 67P/Churyumov-Gerasimenko

Author: Chia-Yu Tzou, Sébastien Gasc, Johan De Keyser, Thierry Sémon, Stephen A. Fuselier, Tamas I. Gombosi, Hans Balsiger, Martin Rubin, Jean-Jacques Berthelier, Kathrin Altwegg, Markus Schuhmann, Nora Hänni, Susanne F. Wampfler, Space Research and Planetary Sciences [Bern) (WP), Physikalisches Institut [Bern], Universität Bern [Bern]-Universität Bern [Bern], Center for Space and Habitability (CSH), University of Bern, PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique (BIRA-IASB), Space Science and Engineering Division [San Antonio], Southwest Research Institute [San Antonio] (SwRI), Department of Climate and Space Sciences and Engineering (CLaSP), University of Michigan [Ann Arbor], and University of Michigan System-University of Michigan System
Subjects: Earth and Planetary Astrophysics (astro-ph.EP), Physics, 0303 health sciences, Atmospheric Science, Comet, FOS: Physical sciences, Coma (optics), Mass spectrometry, 01 natural sciences, Astrobiology, 03 medical and health sciences, [SDU]Sciences of the Universe [physics], 13. Climate action, Space and Planetary Science, Geochemistry and Petrology, 0103 physical sciences, Molecule, 010303 astronomy & astrophysics, Chemical composition, Astrophysics - Earth and Planetary Astrophysics, 030304 developmental biology
Abstract: In 2004, the Rosetta spacecraft was sent to comet 67P/Churyumov-Gerasimenko for the first ever long-term investigation of a comet. After its arrival in 2014, the spacecraft spent more than two years in immediate proximity to the comet. During these two years, the ROSINA Double Focusing Mass Spectrometer (DFMS) onboard Rosetta discovered a coma with an unexpectedly complex chemical composition that included many oxygenated molecules. Determining the exact cometary composition is an essential first step to understanding of the organic rich chemistry in star forming regions and protoplanetary disks that are ultimately conserved in cometary ices. In this study a joint approach of laboratory calibration and space data analysis was used to perform a detailed identification and quantification of CHO-compounds in the coma of 67P/Churyumov-Gerasimenko. The goal was to derive the CHO-compound abundances relative to water for masses up to 100 u. For this study, the May 2015 post-equinox period represent the best bulk abundances of comet 67P/Churyumov-Gerasimenko. A wide variety of CHO-compounds were discovered and their bulk abundances were derived. Finally, these results are compared to abundances of CHO-bearing molecules in other comets, obtained mostly from ground-based observations and modelling., Comment: This document is the unedited Author's version of a Submitted Work that was subsequently accepted for publication in ACS Earth and Space Chemistry, copyright $\copyright$ American Chemical Society after peer review. To access the final edited and published work see https://pubs.acs.org/doi/10.1021/acsearthspacechem.9b00094
Published: 2019

16. Spatio‐temporal patterns of tree growth as related to carbon isotope fractionation in European forests under changing climate

Author: Michael Grabner, Tatjana Boettger, Sławomira Pawełczyk, Marika Haupt, V. R. Switsur, Adomas Vitas, Christina E. Reynolds-Henne, Michel Stievenard, Marek Krąpiec, Luigi Todaro, Neil J. Loader, Eloni Sonninen, Gerhard H. Schleser, Martin Weigl, Monique Pierre, Katja Rinne-Garmston, David Frank, Matthias Saurer, Isabel Dorado-Liñán, Malgorzata Szymaszek, Laia Andreu-Hayles, Tatiana A. Shestakova, Gerhard Helle, Markus Leuenberger, M. Filot, Hamid Marah, Emmi Hilasvuori, John S. Waterhouse, Kerstin Treydte, Anna Pazdur, Antonio Saracino, Jordi Voltas, Valérie Masson-Delmotte, Jan Esper, Rupert Wimmer, Valérie Daux, Zdzisław Bednarz, Högne Jungner, Octavi Planells, Maarit Kalela‐Brundin, Rūtilė Pukienė, Angelo Rita, Frank Berninger, Emilia Gutiérrez, Elżbieta Szychowska‐Kra̧piec, Shestakova, Ta, Voltas, J, Saurer, M, Berninger, F, Esper, J, Andreu-Hayles, L, Daux, V, Helle, G, Leuenberger, M, Loader, Nj, Masson-Delmotte, V, Saracino, Antonio, Waterhouse, J, Schleser, Gh, Bednarz, Z, Boettger, T, Dorado-Liñán, I, Filot, M, Frank, D, Grabner, M, Haupt, M, Hilasvuori, E, Jungner, H, Kalela-Brundin, M, Krąpiec, M, Marah, H, Pawełczyk, S, Pazdur, A, Pierre, M, Planells, O, Pukienė, R, Reynolds-Henne, Ce, Rinne, Kt, Rita, Angelo, Sonninen, E, Stiévenard, M, Switsur, Vr, Szychowska-Krąpiec, E, Szczepanek, M, Todaro, L, Treydte, K, Vitas, A, Weigl, M, Wimmer, R, Gutiérrez, E, Hickler, T., Rinne‐Garmston , Katja T., The Woods Hole Research Center, Woods Hole Oceanographic Institution (WHOI), Department of Crop and Forest Sciences, School of Agrifood and Forestry Science and Engineering (ETSEA), University of Lleida-Agrotecnio Center (UdL-Agrotecnio), Laboratory of Atmospheric Chemistry [Paul Scherrer Institute] (LAC), Paul Scherrer Institute (PSI), Swiss Federal Institute for Forest, Snow and Landscape Research WSL, Department of Forest Sciences [Helsinki], Faculty of Agriculture and Forestry [Helsinki], University of Helsinki-University of Helsinki, Department of Geography [Mainz], Johannes Gutenberg - Universität Mainz (JGU), Tree‐Ring Laboratory, Lamont–Doherty Earth Observatory of Columbia University, Palisades, New York, Laboratoire des Sciences du Climat et de l'Environnement [Gif-sur-Yvette] (LSCE), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ), Géochrononologie Traceurs Archéométrie (GEOTRAC), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ), Glaces et Continents, Climats et Isotopes Stables (GLACCIOS), German Research Centre for Geosciences - Helmholtz-Centre Potsdam (GFZ), Climate and Environmental Physics [Bern] (CEP), Physikalisches Institut [Bern], Universität Bern [Bern]-Universität Bern [Bern], Department of Geography [Swansea], Swansea University, University of Naples Federico II, Anglia Ruskin University (ARU), Institut für Bio- und Geowissenschaften [Jülich], Forschungszentrum Jülich GmbH | Centre de recherche de Juliers, Helmholtz-Gemeinschaft = Helmholtz Association-Helmholtz-Gemeinschaft = Helmholtz Association, Department of Forest Biodiversity, University of Agriculture in Krakow, Department of Isotope Hydrology, Helmholtz Centre for Environmental Research ‒ UFZ, Halle, Germany, Centro de Investigacion Forestal (INIA-CIFOR), Instituto Nacional de Investigación y Tecnología Agraria y Alimentaria = National Institute for Agricultural and Food Research and Technology (INIA), School of Geography and Development and Laboratory of Tree-Ring Research, University of Arizona, University of Natural Resources and Life Sciences (BOKU), Laboratory of Chronology, University of Helsinki, Helsinki, Finland, Forestry Museum, Lycksele, Sweden, AGH University of Science and Technology [Krakow, PL] (AGH UST), Laboratoire d'hydrologie isotopique, CNESTEN, Maroc., Chercheur indépendant, Silesian University of Technology, Department of Biological Evolution, Ecology and Environmental Sciences, University of Barcelona, Barcelona, Spain, The State Scientific Research Institute Nature Research Centre, Vilnius, Lithuania, Oeschger Centre for Climate Change Research (OCCR), University of Bern, Soil Ecosystems, Natural Resources Institute Finland (Luke), University of Basilicata, Department of Radioisotopes, Silesian University of Technology, Gliwice, Poland, Environmental Research Centre, Vytautas Magnus University, Kaunas, Lithuania, Holzforschung Austria, University of Natural Resources and Applied Life Sciences, IFA-Tulln, University of Barcelona, Helsingin yliopisto = Helsingfors universitet = University of Helsinki-Helsingin yliopisto = Helsingfors universitet = University of Helsinki, Johannes Gutenberg - Universität Mainz = Johannes Gutenberg University (JGU), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Universität Bern [Bern] (UNIBE)-Universität Bern [Bern] (UNIBE), University of Naples Federico II = Università degli studi di Napoli Federico II, Laboratory of Tree-Ring Research [University of Arizona] (LTRR), Universität für Bodenkultur Wien = University of Natural Resources and Life [Vienne, Autriche] (BOKU), Natural Resources Institute Finland (LUKE), and Università degli studi della Basilicata [Potenza] (UNIBAS)
Subjects: 0106 biological sciences, Drought stress, 010504 meteorology & atmospheric sciences, [SDE.MCG]Environmental Sciences/Global Changes, Climate change, Fractionation, 010603 evolutionary biology, 01 natural sciences, Panoply, Dendroecology, [SDV.EE.ECO]Life Sciences [q-bio]/Ecology, environment/Ecosystems, Isotope fractionation, [SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistry, Evapotranspiration, ddc:550, Ecosystem, [SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces, environment, ComputingMilieux_MISCELLANEOUS, Ecology, Evolution, Behavior and Systematics, 0105 earth and related environmental sciences, Global and Planetary Change, Ecology, [CHIM.ORGA]Chemical Sciences/Organic chemistry, Tree rings, Carbon isotopes, 15. Life on land, [SDE.ES]Environmental Sciences/Environmental and Society, Tree (data structure), [SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology, 13. Climate action, Isotopes of carbon, [SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/Stratigraphy, [SHS.ENVIR]Humanities and Social Sciences/Environmental studies, Environmental science, carbon isotopes, climate change, dendroecology, drought stress, European forests, latitudinal gradients, Pinus, Quercus, stomatal control, tree rings, European forests
Abstract: Aim The aim was to decipher Europe‐wide spatio‐temporal patterns of forest growth dynamics and their associations with carbon isotope fractionation processes inferred from tree rings as modulated by climate warming. Location Europe and North Africa (30‒70° N, 10° W‒35° E). Time period 1901‒2003. Major taxa studied Temperate and Euro‐Siberian trees. Methods We characterize changes in the relationship between tree growth and carbon isotope fractionation over the 20th century using a European network consisting of 20 site chronologies. Using indexed tree‐ring widths (TRWi), we assess shifts in the temporal coherence of radial growth across sites (synchrony) for five forest ecosystems (Atlantic, boreal, cold continental, Mediterranean and temperate). We also examine whether TRWi shows variable coupling with leaf‐level gas exchange, inferred from indexed carbon isotope discrimination of tree‐ring cellulose (Δ13Ci). Results We find spatial autocorrelation for TRWi and Δ13Ci extending over a maximum of 1,000 km among forest stands. However, growth synchrony is not uniform across Europe, but increases along a latitudinal gradient concurrent with decreasing temperature and evapotranspiration. Latitudinal relationships between TRWi and Δ13Ci (changing from negative to positive southwards) point to drought impairing carbon uptake via stomatal regulation for water saving occurring at forests below 60° N in continental Europe. An increase in forest growth synchrony over the 20th century together with increasingly positive relationships between TRWi and Δ13Ci indicate intensifying impacts of drought on tree performance. These effects are noticeable in drought‐prone biomes (Mediterranean, temperate and cold continental). Main conclusions At the turn of this century, convergence in growth synchrony across European forest ecosystems is coupled with coordinated warming‐induced effects of drought on leaf physiology and tree growth spreading northwards. Such a tendency towards exacerbated moisture‐sensitive growth and physiology could override positive effects of enhanced leaf intercellular CO2 concentrations, possibly resulting in Europe‐wide declines of forest carbon gain in the coming decades. Spanish Government, Grant/Award Number: AGL2015‐68274 ‐C3 ‐3‐R; Sixth Framework Programme, Grant/AwardNumber: EVK2‐2001 ‐00237; Seventh Framework Programme, Grant/AwardNumber: COST ‐STSM ‐ECOST ‐STSM ‐FP1304‐140915‐066395 and ERANET‐Mundus program (Grant agreement 20112573)
Published: 2019

17. Large International Validation of ABSIS and PDAI Pemphigus Severity Scores

Author: Hébert, Vivien, Boulard, Claire, Houivet, Estelle, Lehembre, Sophie, Borradori, Luca, Della, Rocco, Feliciani, Claudio, Fania, Luca, Zambruno, Giovanna, Camaioni, Diana, Didona, Biago, Marinovic, Branka, Schmidt, Enno, Schumacher, Nina, Hü Nefeld 10, Christian, Schanz, Stefan, Kern, Johannes, Hofmann, Silke, Bouyeure, Anne, Picard-Dahan, Catherine, Prost-Squarcioni, Catherine, Caux, Frederic, Alexandre, Marina, Ingen-Housz-Oro, Saskia, Bagot, Martine, Tancrede-Bohin, Emmanuelle, David Bouaziz, Jean, Franck, Nathalie, Vabres, Pierre, Labeille, Bruno, Richard, Marie, Delaporte, Emmanuel, Dupuy, Alain, D'Incan, Michel, Quereux, Gaelle, Skowro, François, Paul, Carle, Livideanu, Cristina, Beylot-Barry, Marie, Doutre, Marie, Avenel-Audran, Martine, Bedane, Christophe, Bernard, Philippe, Machet, Laurent, Maillard, Hervé, Jullien, Denis, Debarbieux, Sebastien, Sassolas, Bruno, Misery, Laurent, Abasq, Claire, Dereure, Olivier, Lagoutte, Philippe, Ferranti, Vincent, Werth, Victoria, Murrell, Dedee, Hertl, Michael, Benichou, Jacques, Joly, Pascal, Duvert Lehembre, Sophie, Della Torre, Rocco, Hünefeld, Christian, Kern, Johannes Steffen, Bouyeure, Anne Charlotte, Bouaziz, Jean David, Richard, Marie Aleth, D’Incan, Michel, Livideanu, Cristina Bulai, Doutre, Marie Sylvie, UNIROUEN - UFR Santé (UNIROUEN UFR Santé), Université de Rouen Normandie (UNIROUEN), Normandie Université (NU)-Normandie Université (NU), Pharmacoepidemiologie et évaluation de l'impact des produits de santé sur les populations, Institut National de la Santé et de la Recherche Médicale (INSERM)-Université Bordeaux Segalen - Bordeaux 2-Université de Rouen Normandie (UNIROUEN), Universität Bern [Bern], Molecular and Cell Biology Laboratory, IDI-IRCCS, Rome, Service de Dermatologie, Hôpital Bichat, AP-HP, Service de dermatologie [Paris], Université Paris Diderot - Paris 7 (UPD7)-Groupe Hospitalier Saint Louis - Lariboisière - Fernand Widal [Paris], Assistance publique - Hôpitaux de Paris (AP-HP) (APHP)-Assistance publique - Hôpitaux de Paris (AP-HP) (APHP), Service de dermatologie [Avicenne], Hôpital Avicenne-Assistance publique - Hôpitaux de Paris (AP-HP) (APHP)-Université Paris 13 (UP13), CHU Henri Mondor, Service de Dermatologie [AP-HP Hôpital Saint Louis, Paris], Université Paris Diderot - Paris 7 (UPD7)-AP-HP Hôpital Saint-Louis, Service de Dermatologie (CHU de Dijon), Centre Hospitalier Universitaire de Dijon - Hôpital François Mitterrand (CHU Dijon), University Hospital of St-Etienne, Department of Dermatology, Université Grenoble Alpes - UFR Pharmacie (UGA UFRP), Université Grenoble Alpes (UGA), Service de dermatologie (CHRU de Lille), Centre Hospitalier Régional Universitaire [Lille] (CHRU Lille), Service de Dermatologie [Rennes], CHU Pontchaillou [Rennes], Imagerie Moléculaire et Stratégies Théranostiques - Clermont Auvergne (IMoST), Institut National de la Santé et de la Recherche Médicale (INSERM)-Université Clermont Auvergne (UCA), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Service de dermatologie [Bordeaux], Université Bordeaux Segalen - Bordeaux 2-CHU Bordeaux [Bordeaux]-Hôpital Haut-Lévêque [CHU Bordeaux], CHU Bordeaux [Bordeaux], Département de Dermatologie, Centre Hospitalier Universitaire d'Angers (CHU Angers), PRES Université Nantes Angers Le Mans (UNAM)-PRES Université Nantes Angers Le Mans (UNAM), Service de Dermatologie [CHU Limoges], CHU Limoges, Club Rhumatismes et Inflammation, Service de Dermatologie, Centre Hospitalier Sud, Hospices Civils, Lyon, Département de Médecine Interne et Pneumologie [Brest] (DMIP - Brest), Centre Hospitalier Régional Universitaire de Brest (CHRU Brest), Service de dermatologie (Dermato - BREST), Centre Hospitalier Régional Universitaire [Montpellier] (CHRU Montpellier), Génétique médicale et fonctionnelle du cancer et des maladies neuropsychiatriques, Normandie Université (NU)-Normandie Université (NU)-Institut National de la Santé et de la Recherche Médicale (INSERM), Physiopathologie et biothérapies des maladies inflammatoires et autoimmunes, Seventh Framework Programme, French Society of Dermatology, Centre Hospitalier Universitaire de Reims (CHU Reims), Immuno-Régulation dans les Maladies Auto-Immunes Inflammatoires et le Cancer - EA 7509 (IRMAIC), Université de Reims Champagne-Ardenne (URCA), CHU Rouen, Normandie Université (NU), Service de dermatologie [Rouen], Normandie Université (NU)-Normandie Université (NU)-Université de Rouen Normandie (UNIROUEN), Unité de biostatistiques [Rouen], Service de Dermatologie [Rouen], Hôpital Charles Nicolle [Rouen]-CHU Rouen, Assistance publique - Hôpitaux de Paris (AP-HP) (APHP)-Groupe Hospitalier Saint Louis - Lariboisière - Fernand Widal [Paris]-Université Paris Diderot - Paris 7 (UPD7), Université Paris 13 (UP13)-Assistance publique - Hôpitaux de Paris (AP-HP) (APHP)-Hôpital Avicenne, Institut Mondor de recherche biomédicale (IMRB), Institut National de la Santé et de la Recherche Médicale (INSERM)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12), L'Oréal recherche et innovation, L'Oréal, Institut de Génétique et Développement de Rennes (IGDR), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-IFR140-Centre National de la Recherche Scientifique (CNRS), Service de Dermatologie, Hôtel-Dieu, Centre de Recherche en Cancérologie / Nantes - Angers (CRCNA), Centre hospitalier universitaire de Nantes (CHU Nantes)-Faculté de Médecine d'Angers-Centre Hospitalier Universitaire d'Angers (CHU Angers), PRES Université Nantes Angers Le Mans (UNAM)-PRES Université Nantes Angers Le Mans (UNAM)-Centre National de la Recherche Scientifique (CNRS)-Hôpital Laennec-Institut National de la Santé et de la Recherche Médicale (INSERM)-Hôtel-Dieu de Nantes, Université Toulouse III - Paul Sabatier (UPS), Immunodermatologie, Cytokines, Cancer - EA 7319 (ICA), Service de dermatologie (CHRU de Tours), Centre Hospitalier Régional Universitaire de Tours (CHRU TOURS), INSERM U1234, Bordeaux population health (BPH), Université de Bordeaux (UB)-Institut de Santé Publique, d'Épidémiologie et de Développement (ISPED)-Institut National de la Santé et de la Recherche Médicale (INSERM), Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP), Université Paris 13 (UP13)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Hôpital Avicenne [AP-HP], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP), Université Paris Diderot - Paris 7 (UPD7)-Hopital Saint-Louis [AP-HP] (AP-HP), Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Service de Dermatologie [Rennes] = Dermatology [Rennes], Imagerie Moléculaire et Stratégies Théranostiques (IMoST), Institut National de la Santé et de la Recherche Médicale (INSERM)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020]), Pathogénèse et contrôle des infections chroniques (PCCI), Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre Hospitalier Universitaire de Montpellier (CHU Montpellier )-Université de Montpellier (UM), Institut National de la Santé et de la Recherche Médicale (INSERM)-Université de Rouen Normandie (UNIROUEN), Université Bordeaux Segalen - Bordeaux 2-Université de Rouen Normandie (UNIROUEN), Universität Bern [Bern] (UNIBE), IDI-IRCCS [Roma, Italy], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Université Paris Diderot - Paris 7 (UPD7)-Groupe Hospitalier Saint Louis - Lariboisière - Fernand Widal [Paris], CHU Henri Mondor [Créteil], Service de Dermatologie [CHU Saint-Etienne], Centre Hospitalier Universitaire de Saint-Etienne [CHU Saint-Etienne] (CHU ST-E)-Université Jean Monnet - Saint-Étienne (UJM), Université de Toulouse (UT), and Centre Hospitalier Régional Universitaire [Montpellier] (CHRU Montpellier)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université de Montpellier (UM)
Subjects: 0301 basic medicine, Autoimmune Bullous Skin Disorder Intensity Score, Intraclass correlation, [SDV]Life Sciences [q-bio], intraclass correlation coefficient, Autoimmunity, PV, Validation Studies as Topic, Severity of Illness Index, Biochemistry, PDAI, 0302 clinical medicine, Medicine, DLQI, Pemphigus foliaceus, Skin, integumentary system, Desmoglein 1, PGA, CI, 3. Good health, ABSIS, month, 030220 oncology & carcinogenesis, PF, medicine.medical_specialty, pemphigus vulgaris, [SDV.CAN]Life Sciences [q-bio]/Cancer, Dermatology, 03 medical and health sciences, Dermatology Quality of Life Index, Internal medicine, Severity of illness, Humans, In patient, pemphigus foliaceus, Molecular Biology, Autoantibodies, Pemphigus severity scores, ICC, business.industry, Pemphigus vulgaris, Cell Biology, medicine.disease, Confidence interval, Moderate extent, Pemphigus Disease Area Index, Pemphigus, 030104 developmental biology, confidence interval, Physician Global Assessment, business, [SDV.MHEP.DERM]Life Sciences [q-bio]/Human health and pathology/Dermatology, [SDV.MHEP]Life Sciences [q-bio]/Human health and pathology
Abstract: IF 6.448 (2017); International audience; The Pemphigus Disease Area Index (PDAI) and Autoimmune Bullous Skin Disorder Intensity-Score (ABSIS) scores have been proposed to provide an objective measure of pemphigus activity. These scores have been evaluated only on already treated patients mainly with mild to moderate activity. The objective was to assess the interrater reliability of ABSIS and PDAI scores and their correlation with other severity markers in a large international study. Consecutive patients with newly diagnosed pemphigus were enrolled in 31 centers. Severity scores were recorded during a 24-month period by the same two blinded investigators. Serum was collected at each visit for ELISA measurement of anti-desmoglein antibodies. The intraclass correlation coefficient (ICC) and Spearman rank correlation coefficient were calculated. A total of 116 patients with pemphigus vulgaris (n = 84) or pemphigus foliaceus (n = 32) were included. At baseline, the ABSIS and PDAI ICCs were 0.90 (95% confidence interval [CI] = 0.85-0.93), and 0.91(95% CI = 0.87-0.94), respectively. The ICCs for PDAI were higher in moderate and extensive pemphigus (ICC = 0.82, 95% CI = 0.63-0.92 and ICC = 0.80, 95% CI = 0.62-0.90, respectively) than in patients with intermediate (significant) extent (ICC = 0.50, 95% CI = 0.27-0.68). Conversely, the ICCs for ABSIS were lower in patients with moderate extent (ICC = 0.44, 95% CI = 0.004-0.74) than in those with intermediate or extensive forms, (ICC = 0.69, 95% CI = 0.51-0.81 and ICC = 0.75, 95% CI = 0.51-0.88, respectively). During patients' follow-up, the ICCs of both ABSIS and PDAI scores remained higher than 0.70. ABSIS and PDAI skin (r = 0.71 and r = 0.75) but not mucosal (r = 0.32 and r = 0.37) subscores were correlated with the evolution of anti-DSG1 and anti-DSG3 ELISA values, respectively. ABSIS and PDAI scores are robust tools to accurately assess pemphigus activity.
Published: 2019

18. Perturbers: SPHERE detection limits to planetary-mass companions in protoplanetary disks

Author: Ruobing Dong, Maud Langlois, Joany Andreina Manjarres Ramos, R. van Boekel, S. Jorquera, Myriam Benisty, E. L. Rickman, R. Asensio-Torres, M. Villenave, Antonio Garufi, Gael Chauvin, Th. Henning, L. Gluck, Markus Janson, Raffaele Gratton, A. Pavlov, C. Desgrange, Gabriel-Dominique Marleau, Faustine Cantalloube, P. Pinilla, Thierry Fusco, Markus Feldt, Dino Mesa, C. Bergez-Casalou, M. Keppler, Tomas Stolker, Judit Szulágyi, François Ménard, Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, INAF - Osservatorio Astronomico di Padova (OAPD), Istituto Nazionale di Astrofisica (INAF), INAF - Osservatorio Astrofisico di Arcetri (OAA), Laboratoire Franco-Chilien d'Astronomie (LFCA), Universidad de Chile = University of Chile [Santiago] (UCHILE)-Pontificia Universidad Católica de Chile (UC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Universidad de Concepción - University of Concepcion [Chile], Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, Institute for Particle Physics and Astrophysics [ETH Zürich] (IPA), Department of Physics [ETH Zürich] (D-PHYS), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich)- Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), University of Victoria [Canada] (UVIC), Institut für Astronomie und Astrophysik [Tübingen] (IAAT), Eberhard Karls Universität Tübingen = Eberhard Karls University of Tuebingen, Physikalisches Institut [Bern], Universität Bern [Bern] (UNIBE), Ecole normale supérieure de Lyon (Ens Lyon), Stockholm University, Centre de Recherche Astrophysique de Lyon (CRAL), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Observatoire Astronomique de l'Université de Genève (ObsGE), Université de Genève = University of Geneva (UNIGE), European Space Agency (Baltimore) Space Telescope Science Institute (ESA), Leiden Observatory [Leiden], Universiteit Leiden, Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), DOTA, ONERA, Université Paris Saclay [Châtillon], ONERA-Université Paris-Saclay, Universidad de Concepción [Chile]-Pontificia Universidad Católica de Chile (UC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Universidad de Chile, Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA), Universität Bern [Bern], École normale supérieure - Lyon (ENS Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Université de Genève (UNIGE), Universiteit Leiden [Leiden], and Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES)
Subjects: Protoplanetary disks, Continuum (design consultancy), FOS: Physical sciences, Astrophysics, 01 natural sciences, Luminosity, [SPI]Engineering Sciences [physics], High angular resolution, Image processing, Planet, 0103 physical sciences, Solar and Stellar Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics::Galaxy Astrophysics, protoplanetary disks, planet-disk interactions, planets and satellites, detection, techniques, high angular resolution, image processing, Earth and Planetary Astrophysics (astro-ph.EP), Physics, [PHYS]Physics [physics], 010308 nuclear & particles physics, Planets and Satellites, Astronomy and Astrophysics, Planets and satellites: detection, Techniques, Detection, Astrophysics - Solar and Stellar Astrophysics, 13. Climate action, Space and Planetary Science, [SDU]Sciences of the Universe [physics], Hill sphere, Instrumentation and Methods for Astrophysics, Substructure, Millimeter, Astrophysics::Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Planetary mass, Order of magnitude, Planet-disk interactions, Astrophysics - Earth and Planetary Astrophysics
Abstract: The detection of a wide range of substructures such as rings, cavities and spirals has become a common outcome of high spatial resolution imaging of protoplanetary disks, both in the near-infrared scattered light and in the thermal millimetre continuum emission. The most frequent interpretation of their origin is the presence of planetary-mass companions perturbing the gas and dust distribution in the disk (perturbers), but so far the only bona-fide detection has been the two giant planets around PDS 70. Here, we collect a sample of 15 protoplanetary disks showing substructures in SPHERE scattered light images and present a homogeneous derivation of planet detection limits in these systems. We also estimate the mass of these perturbers through a Hill radius prescription and a comparison to ALMA data. Assuming that one single planet carves each substructure in scattered light, we find that more massive perturbers are needed to create gaps within cavities than rings, and that we might be close to a detection in the cavities of RX J1604, RX J1615, Sz Cha, HD 135344B and HD 34282. We reach typical mass limits in these cavities of 3-10 Mjup. For planets in the gaps between rings, we find that the detection limits of SPHERE are about an order of magnitude away in mass, and that the gaps of PDS 66 and HD 97048 seem to be the most promising structures for planet searches. The proposed presence of massive planets causing spiral features in HD 135344B and HD 36112 are also within SPHERE's reach assuming hot-start models.These results suggest that current detection limits are able to detect hot-start planets in cavities, under the assumption that they are formed by a single perturber located at the centre of the cavity. More realistic planet mass constraints would help to clarify whether this is actually the case, which might point to perturbers not being the only way of creating substructures., 26 pages, 33 figures, accepted for publication in A&A
Published: 2021

19. Functional rarity and evenness are key facets of biodiversity to boost multifunctionality

Author: Johannes H. C. Cornelissen, Victoria Ochoa, Sonia Ruiz, Norma Salinas, Hugo Saiz, Jun-Tao Wang, Sergio Asensio, Carmen García, Pablo García-Palacios, Rubén Milla, Marina Dacal, Fernando T. Maestre, Brajesh K. Singh, Vincent Maire, Yoann Le Bagousse-Pinguet, Beatriz Gozalo, Lucas Deschamps, Nicolas Gross, Universidad Rey Juan Carlos [Madrid] (URJC), Institut méditerranéen de biodiversité et d'écologie marine et continentale (IMBE), Avignon Université (AU)-Aix Marseille Université (AMU)-Institut de recherche pour le développement [IRD] : UMR237-Centre National de la Recherche Scientifique (CNRS), Unité Mixte de Recherche sur l'Ecosystème Prairial - UMR (UREP), VetAgro Sup - Institut national d'enseignement supérieur et de recherche en alimentation, santé animale, sciences agronomiques et de l'environnement (VAS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Universität Bern [Bern] (UNIBE), Universidad de Alicante, Vrije Universiteit Brussel (VUB), Université du Québec à Trois-Rivières (UQTR), Consejo Superior de Investigaciones Científicas [Spain] (CSIC), Peruvian University of Applied Sciences, Western Sydney University, Universidad de Alicante. Departamento de Ecología, Universidad de Alicante. Instituto Multidisciplinar para el Estudio del Medio 'Ramón Margalef', Systems Ecology, Universität Bern [Bern], British Ecological Society, European Research Council, European Commission, Ministerio de Economía y Competitividad (España), Generalitat Valenciana, Ministerio de Educación, Cultura y Deporte (España), Australian Research Council, and Ministerio de Ciencia, Innovación y Universidades (España)
Subjects: 0106 biological sciences, 0301 basic medicine, Trait distributions, Range (biology), Rare species, Biodiversity, litter decomposition, Biology, plant pathogens, Nutrient cycling, complex species assemblages, 010603 evolutionary biology, 01 natural sciences, Complex species assemblages | litter decomposition | nutrient cycling | plant pathogens | trait distributions, Carbon Cycle, Complex species assemblages, 03 medical and health sciences, Abundance (ecology), trait distributions, Ecosystem, Biomass, Plant Physiological Phenomena, Multidisciplinary, Ecology, Litter decomposition, nutrient cycling, Biological Sciences, Ecología, 15. Life on land, Plant disease, Plant Leaves, 030104 developmental biology, Trait, Species evenness, Plant pathogens, [SDE.BE]Environmental Sciences/Biodiversity and Ecology
Abstract: The functional traits of organisms within multispecies assemblages regulate biodiversity effects on ecosystem functioning. Yet how traits should assemble to boost multiple ecosystem functions simultaneously (multifunctionality) remains poorly explored. In a multibiome litter experiment covering most of the global variation in leaf trait spectra, we showed that three dimensions of functional diversity (dispersion, rarity, and evenness) explained up to 66% of variations in multifunctionality, although the dominant species and their traits remained an important predictor. While high dispersion impeded multifunctionality, increasing the evenness among functionally dissimilar species was a key dimension to promote higher multifunctionality and to reduce the abundance of plant pathogens. Because too-dissimilar species could have negative effects on ecosystems, our results highlight the need for not only diverse but also functionally even assemblages to promote multifunctionality. The effect of functionally rare species strongly shifted from positive to negative depending on their trait differences with the dominant species. Simultaneously managing the dispersion, evenness, and rarity in multispecies assemblages could be used to design assemblages aimed at maximizing multifunctionality independently of the biome, the identity of dominant species, or the range of trait values considered. Functional evenness and rarity offer promise to improve the management of terrestrial ecosystems and to limit plant disease risks., This work was funded by the British Ecological Society (SR17\1297 grant, PI: P.G.-P.) and by the European Research Council (ERC Grant Agreement #647038, BIODESERT, PI: F.T.M.). Y.L.B.-P. was supported by a Marie Sklodowska-Curie Actions Individual Fellowship within the European Program Horizon 2020 (DRYFUN Project #656035). H.S. was supported by a Juan de la Cierva-Formación grant from the Span ish Ministry of Economy and Competitiveness (FJCI-2015-26782). F.T.M. and S.A. were supported from the Generalitat Valenciana (CIDEGENT/ 2018/041). M.D. was supported by a Formación del Profesorado Universi tario (FPU) fellowship from the Spanish Ministry of Education, Culture and Sports (FPU-15/00392). S.A. was supported by the Spanish MINECO for financial support via the DIGGING_DEEPER project through the 2015 to 2016 BiodivERsA3/FACCE‐JPI joint call for research proposals. B.K.S. re search on biodiversity-ecosystem functions was supported by the Austra lian Research Council (DP170104634 and DP190103714). P.G.-P. was supported by a Ramón y Cajal grant from the Spanish Ministry of Science and Innovation (RYC2018-024766-I). R.M. was supported by MINECO (Grants CGL2014-56567-R and CGL2017-83855-R)
Published: 2021

20. SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo

Author: Hans Nilsson, R. S. Gurnee, Wolfgang Baumjohann, Howard Smith, Menelaos Sarantos, Mark Phillips, Iannis Dandouras, S. Shuvalov, V. Grishin, D. Moissenko, Stavro Ivanovski, Johan Svensson, John Hayes, Markus Fränz, Stefano Orsini, Francesco Lazzarotto, S. Persyn, Stefano Selci, Rosemary M. Killen, S. M. P. McKenna-Lawlor, V. Mangano, Diana Gamborino, Sándor Szalai, B. Trantham, P. Wilson, M. Oja, M. Cantatore, François Leblanc, Peter Wurz, H. Jeszenszky, Dominique Delcourt, Chuanfei Dong, Helmut Lammer, A. Shestakov, A. Aronica, A. Loose, S. Barabash, H. Fischer, E. De Angelis, M. Famá, M. Wieser, C. Nunez, Harald Krüger, Kerrington D. Smith, George C. Ho, G. Laky, L. Cremonesi, Mats Holmström, Manuel Grande, C. Kürbisch, Raffaella Noschese, D. Toublanc, Fabio Camozzi, C. P. Escoubet, L. Szalai, Francesco Mattioli, P. Wahlstroem, D. Maschietti, James A. Slavin, N. Vertolli, L. Colasanti, Frederic Allegrini, F. Giner, Jean-Jacques Berthelier, W. C. Gibson, Roberto Leoni, Dennis Haggerty, Stefano Massetti, Fabrizio Nuccilli, R. Wallner, S. Zampieri, Anna Milillo, Magda Delva, G. Fremuth, A. M. Di Lellis, Raymond Goldstein, Sara Cibella, Esa Kallio, Greg Miller, Walter Schmidt, Alessandro Gaggero, J. A. Scheer, M. I. Desai, Philippe Garnier, U. Bührke, Shahab Fatemi, Karoly Kecskemety, D. Brienza, Marco D'Alessandro, Adrian Kazakov, M. Leichtfried, Karoly Szego, Stefano Livi, A. Olivieri, F. Tominetti, A. D. Jacques, Alfredo Morbidini, Istvan Dr Horvath, Nikolaos Paschalidis, Daniele Piazza, Ioannis A. Daglis, Alessandro Mura, C. Urdiales, Herbert Lichtenegger, Christina Plainaki, Jim M. Raines, J. Balaz, Rosanna Rispoli, K. C. Hsieh, Kanako Seki, F. Leblanc, Roberto Sordini, J. Ryno, O. L. Vaisberg, A. Varsani, M. D. Bush, Klaus Torkar, M. Ferris, G. Cremonese, Robert E. Johnson, Norbert Krupp, Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS), Istituto Nazionale di Astrofisica (INAF), Southwest Research Institute [San Antonio] (SwRI), Department of Climate and Space Sciences and Engineering (CLaSP), University of Michigan [Ann Arbor], University of Michigan System-University of Michigan System, Space Research Institute of Austrian Academy of Sciences (IWF), Austrian Academy of Sciences (OeAW), Swedish Institute of Space Physics [Kiruna] (IRF), Italian Space Agency, Johns Hopkins University Applied Physics Laboratory [Laurel, MD] (APL), NASA Goddard Space Flight Center (GSFC), Physics Institute [Bern], University of Bern, HELIOS - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Department of Electronics and Nanoengineering [Espoo], School of Electrical Engineering [Aalto Univ], Aalto University-Aalto University, Space Technology Ireland Limited, Wigner Research Centre for Physics [Budapest], Hungarian Academy of Sciences (MTA), Space Research Institute of the Russian Academy of Sciences (IKI), Russian Academy of Sciences [Moscow] (RAS), Department of Physics [Athens], National and Kapodistrian University of Athens (NKUA), Princeton Plasma Physics Laboratory (PPPL), Princeton University, Research and Scientific Support Department, ESTEC (RSSD), European Space Research and Technology Centre (ESTEC), Agence Spatiale Européenne = European Space Agency (ESA)-Agence Spatiale Européenne = European Space Agency (ESA), Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research (MPS), Max-Planck-Gesellschaft, INAF - Osservatorio Astronomico di Trieste (OAT), Institut für Weltraumforschung = Space Research institute [Graz] (IWF), Osterreichische Akademie der Wissenschaften (ÖAW), Laboratory for Atmospheric and Space Physics [Boulder] (LASP), University of Colorado [Boulder], CNR Institute for Photonics and Nanotechnologies (IFN), National Research Council of Italy | Consiglio Nazionale delle Ricerche (CNR), INAF - Osservatorio Astronomico di Padova (OAPD), Istituto di Struttura della Materia (CNR-ISM), Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Comisión Nacional de Energía Atómica [ARGENTINA] (CNEA), Physikalisches Institut [Bern], Universität Bern [Bern] (UNIBE), Institute of Mathematical and Physical Sciences [Aberystwyth], University of Wales, University of Arizona, Department of Materials Science and Engineering [Charlottesville] (MS), University of Virginia, Laboratoire de Physique des Plasmas (LPP), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École polytechnique (X)-Sorbonne Université (SU)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Finnish Meteorological Institute (FMI), Department of Earth and Planetary Science [Tokyo], Graduate School of Science [Tokyo], The University of Tokyo (UTokyo)-The University of Tokyo (UTokyo), EISCAT Scientific Association [Sweden], Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), European Space Agency (ESA)-European Space Agency (ESA), Max-Planck-Institut für Sonnensystemforschung (MPS), Institut für Weltraumforschung [Graz] (IWF), Consiglio Nazionale delle Ricerche [Roma] (CNR), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National d’Études Spatiales [Paris] (CNES), Universität Bern [Bern], University of Virginia [Charlottesville], The University of Tokyo (UTokyo), National Institute for Astrophysics, Southwest Research Institute, Austrian Academy of Sciences, Uppsala University, Agenzia Spaziale Italiana, Johns Hopkins Applied Physics Laboratory, NASA Goddard Space Flight Center, University of Michigan, Ann Arbor, UMR7095, IRAP, Department of Electronics and Nanoengineering, Space Technology Ireland, Hungarian Academy of Sciences, Space Research Institute of the Russian Academy of Sciences, National and Kapodistrian University of Athens, United States Department of Energy, European Space Research and Technology Centre, Max Planck Institute for Solar System Research, Osservatorio Astronomico di Trieste, AMDL Srl, University of Colorado Boulder, Slovak Academy of Sciences, National Research Council of Italy, INAF - Osservatorio Astronomico di Padova, Université d'Orléans, Comisión Nacional de Energía Atómica, Aberystwyth University, Université Paris-Saclay, Finnish Meteorological Institute, Tofwerk AG, The University of Tokyo, EISCAT Headquarters, Aalto-yliopisto, and Aalto University
Subjects: 010504 meteorology & atmospheric sciences, chemistry.chemical_element, 7. Clean energy, 01 natural sciences, Article, Astrobiology, law.invention, Particle instrumentation, Mercury’s environment, Orbiter, Interplanetary dust cloud, law, 0103 physical sciences, Calibration, BepiColombo space mission, Neutral particle, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, Spacecraft, business.industry, 520 Astronomy, Astronomy and Astrophysics, 620 Engineering, Mercury (element), Solar wind, Planetary science, chemistry, Space and Planetary Science, [SDU]Sciences of the Universe [physics], Physics::Space Physics, Environmental science, Astrophysics::Earth and Planetary Astrophysics, business
Abstract: The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at Mercury as well as their interactions with solar wind, solar radiation, and interplanetary dust. The particle instrument suite SERENA (Search for Exospheric Refilling and Emitted Natural Abundances) is flying in space on-board the BepiColombo Mercury Planetary Orbiter (MPO) and is the only instrument for ion and neutral particle detection aboard the MPO. It comprises four independent sensors: ELENA for neutral particle flow detection, Strofio for neutral gas detection, PICAM for planetary ions observations, and MIPA, mostly for solar wind ion measurements. SERENA is managed by a System Control Unit located inside the ELENA box. In the present paper the scientific goals of this suite are described, and then the four units are detailed, as well as their major features and calibration results. Finally, the SERENA operational activities are shown during the orbital path around Mercury, with also some reference to the activities planned during the long cruise phase.
Published: 2021

21. Impact on survival through consolidation radiotherapy for diffuse large B-cell lymphoma: a comprehensive meta-analysis

Author: Thierry Lamy de la Chapelle, Sabrina Jegerlehner, Urban Novak, Sven Trelle, Martin D. Berger, Codruta Ionescu, Annina Elisabeth Büchi, Chard-Hutchinson, Xavier, Bern University Hospital [Berne] (Inselspital), Universität Bern [Bern] (UNIBE), CHU Pontchaillou [Rennes], Microenvironment, Cell Differentiation, Immunology and Cancer (MICMAC), Université de Rennes (UR)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Structure Fédérative de Recherche en Biologie et Santé de Rennes ( Biosit : Biologie - Santé - Innovation Technologique ), Universität Bern [Bern], Université de Rennes 1 (UR1), and Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Structure Fédérative de Recherche en Biologie et Santé de Rennes ( Biosit : Biologie - Santé - Innovation Technologique )
Subjects: 0301 basic medicine, Oncology, medicine.medical_specialty, medicine.medical_treatment, [SDV]Life Sciences [q-bio], 610 Medicine & health, Article, 03 medical and health sciences, 0302 clinical medicine, Internal medicine, Positron Emission Tomography Computed Tomography, Antineoplastic Combined Chemotherapy Protocols, medicine, Clinical endpoint, Humans, Proportional Hazards Models, Chemotherapy, business.industry, Hazard ratio, Hematology, medicine.disease, 3. Good health, Lymphoma, Radiation therapy, [SDV] Life Sciences [q-bio], 030104 developmental biology, 030220 oncology & carcinogenesis, Meta-analysis, Rituximab, Lymphoma, Large B-Cell, Diffuse, business, Diffuse large B-cell lymphoma, medicine.drug
Abstract: Rituximab has improved response rates and overall survival in diffuse large B-cell lymphoma. Radiotherapy is an effective treatment modality for lymphomas, but there is uncertainty on its use as consolidation after chemo-immunotherapy mainly in advanced stages. We evaluated its efficacy with a comprehensive meta-analysis and a systematic search of Pubmed, Embase, Cochrane, and abstracts from the American Society of Clinical Oncology, American Society of Hematology, European Society for Medical Oncology and American Society of Radiation Oncology published from June 1966 and December 2018. We identified 11 trials that evaluated consolidation radiotherapy following chemotherapy in a randomized fashion in 4,584 patients. The primary endpoint of this meta-analysis was progression-free survival (PFS). As three of the 11 trials were retracted, this data is based on 2,414 patients. For the primary endpoint, PFS, we found a hazard ratio (HR) 0.77 (95% Confidence Interval [CI]: 0.51-1.17), pooled (tau2: 0.25; I2: 85%), and a HR 0.80 (95% CI: 0.53-1.21), pooled in a bivariate metaanalysis and for the secondary endpoint, overall survival, a HR 0.93 (range, 0.61-1.40), pooled (tau2: 0.25; I2: 74%) and a HR 0.86 (95% CI: 0.58-1.27) in a bivariate meta-analysis. The lack of benefit did not change over time (P=0.95 (tau2: 0.32; I2: 88%), and was also absent for PFS when stratifying for i) chemotherapy, ii) the use of rituximab, iii) age, iv) the dose of radiotherapy and v) application to patients in complete remission with bulky disease. None of the trials used a positron emission tomography- guided approach. This meta-analysis revealed no survival benefit when consolidation radiotherapy is given to unselected diffuse large Bcell lymphoma patients following chemotherapy. These results need to be considered in future trials in the positron emission tomography-computed tomography era.
Published: 2021

22. The Late Palaeozoic Ice Age unconformity in southern Namibia viewed as a patchwork mosaic

Author: Roland Mundil, Isabel P. Montañez, Guilhem Amin Douillet, Daniel Paul Le Heron, Pierre Dietrich, Christoph Kettler, Neil Griffis, David A. Osleger, Axel Hofmann, Universität Wien, University of California [Davis] (UC Davis), University of California, Géosciences Rennes (GR), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Rennes (OSUR)-Centre National de la Recherche Scientifique (CNRS), University of Johannesburg (UJ), Institut für Geologie [Bern], Universität Bern [Bern], Berkeley Geochronology Center (BGC), South Africa–Austria joint project of the National Research Foundation (NRF), Österreichischer Austauschdienst (OEAD Project no. ZA 08/2019), University of California (UC), Université de Rennes (UR)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Rennes (OSUR), Université de Rennes (UR)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Centre National de la Recherche Scientifique (CNRS), University of Johannesburg [South Africa] (UJ), and Universität Bern [Bern] (UNIBE)
Subjects: glacial, 010504 meteorology & atmospheric sciences, Late Palaeozoic, Stratigraphy, Ice stream, Environmental Science (miscellaneous), 010502 geochemistry & geophysics, Oceanography, 01 natural sciences, Unconformity, Paleontology, Ice age, Late Paleozoic, Glacial period, 0105 earth and related environmental sciences, geography, geography.geographical_feature_category, ice sheets, Geology, Fold (geology), 15. Life on land, Gondwana, [SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/Stratigraphy, Siliciclastic, Ice sheet
Abstract: International audience; The expansion of ice masses across southern Africa during the Late Palaeozoic Ice Age has been known for 150 years, including the distribution of upland areas in controlling the configuration of glaciation. In Accepted Article This article is protected by copyright. All rights reserved Namibia, increasing attention has focussed on long and deep palaeovalley networks in the Kaokoland region in the north, but comparatively little work has been attempted in the topographically subdued plains of the south, in the Aranos and Karasburg basins. The desert terrain of the Aranos area exposes diamictites of the Dwyka Group discontinuously over about 300 km, extending further south to the Karasburg area at the Namibian-South African border along the Orange River. Whilst examined at a stratigraphic level, the nature of the contact between the Dwyka glacial rocks and underlying lithologies has not been systematically investigated. This paper presents the results from fieldwork in austral winter 2019, in which a highly varying basal contact is described that records the processes of growth, flow and expansion of ice masses across this part of Gondwana. At the basin margins, subglacially-produced unconformities exhibit classic glacially striated pavements on indurated bedrock. In comparison, the basal subglacial unconformity in the more basinward regions is characterised by soft-sediment striated surfaces and deformation. In the Aranos Basin, soft-sediment shear zones originated in the subglacial environment. This type of subglacial unconformity developed over well differentiated, unconsolidated, siliciclastic materials. Where ice advanced over more poorly sorted material or cannibalised pre-existing diamictites, "boulder-pavements" recognized as single clast-thick boulder-dominated intervals formed. Importantly, these boulder-pavements are enriched in clasts, which were facetted and striated in-situ by overriding ice. By integrating measurements of striation orientations, fold vergence and palaeocurrent information, former ice flow pathways can potentially be reconstructed over a wide area.
Published: 2021

23. The CHEOPS mission

Author: Benz, W., Broeg, C., Fortier, A., Rando, N., Beck, T., Beck, M., Queloz, D., Ehrenreich, D., Maxted, P. F. L., Isaak, K. G., Billot, N., Alibert, Y., Alonso, R., António, C., Asquier, J., Bandy, T., Bárczy, T., Barrado, D., Barros, S. C. C., Baumjohann, W., Bekkelien, A., Bergomi, M., Biondi, F., Bonfils, X., Borsato, L., Brandeker, A., Busch, M.-D., Cabrera, J., Cessa, V., Charnoz, S., Chazelas, B., Collier Cameron, A., Corral Van Damme, C., Cortes, D., Davies, M. B., Deleuil, M., Deline, A., Delrez, L., Demangeon, O., Demory, B. O., Erikson, A., Farinato, J., Fossati, L., Fridlund, M., Futyan, D., Gandolfi, D., Garcia Munoz, A., Gillon, M., Guterman, P., Gutierrez, A., Hasiba, J., Heng, K., Hernandez, E., Hoyer, S., Kiss, L. L., Kovacs, Z., Kuntzer, T., Laskar, J., Lecavelier des Etangs, A., Lendl, M., López, A., Lora, I., Lovis, C., Lüftinger, T., Magrin, D., Malvasio, L., Marafatto, L., Michaelis, H., de Miguel, D., Modrego, D., Munari, M., Nascimbeni, V., Olofsson, G., Ottacher, H., Ottensamer, R., Pagano, I., Palacios, R., Pallé, E., Peter, G., Piazza, D., Piotto, G., Pizarro, A., Pollaco, D., Ragazzoni, R., Ratti, F., Rauer, H., Ribas, I., Rieder, M., Rohlfs, R., Safa, F., Salatti, M., Santos, N. C., Scandariato, G., Ségransan, D., Simon, A. E., Smith, A. M. S., Sordet, M., Sousa, S. G., Steller, M., Szabó, G. M., Szoke, J., Thomas, N., Tschentscher, M., Udry, S., Van Grootel, V., Viotto, V., Walter, I., Walton, N. A., Wildi, F., Wolter, D., Fundação para a Ciência e a Tecnologia (Portugal), Ministerio de Ciencia, Innovación y Universidades (España), Generalitat de Catalunya, European Commission, University of St Andrews. School of Physics and Astronomy, University of St Andrews. St Andrews Centre for Exoplanet Science, Benz, W. [0000-0001-7896-6479], Apollo - University of Cambridge Repository, Physikalisches Institut [Bern], Universität Bern [Bern], Observatoire Astronomique de l'Université de Genève (ObsGE), Université de Genève (UNIGE), School of Physics and Astronomy [Cardiff], Cardiff University, Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA), Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Universität Bern [Bern] (UNIBE), Université de Genève = University of Geneva (UNIGE), and Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France
Subjects: 530 Physics, media_common.quotation_subject, FOS: Physical sciences, 01 natural sciences, 7. Clean energy, law.invention, 010309 optics, Telescope, Planet, law, 0103 physical sciences, QB Astronomy, Astrophysics::Solar and Stellar Astrophysics, CHEOPS, 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), QB600, QC, Astrophysics::Galaxy Astrophysics, media_common, QB, Earth and Planetary Astrophysics (astro-ph.EP), High-precision transit photometry, 520 Astronomy, Exoplanets, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Astronomy and Astrophysics, Small mission, 3rd-DAS, 620 Engineering, Exoplanet, Space observatory, Stars, Photometry (astronomy), QC Physics, Space and Planetary Science, Sky, [SDU]Sciences of the Universe [physics], Physics::Space Physics, Satellite, Original Article, Astrophysics::Earth and Planetary Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Instrumentation and Methods for Astrophysics, Geology, Astrophysics - Earth and Planetary Astrophysics
Abstract: Benz, W., et al., The CHaracterising ExOPlanet Satellite (CHEOPS) was selected on October 19, 2012, as the first small mission (S-mission) in the ESA Science Programme and successfully launched on December 18, 2019, as a secondary passenger on a Soyuz-Fregat rocket from Kourou, French Guiana. CHEOPS is a partnership between ESA and Switzerland with important contributions by ten additional ESA Member States. CHEOPS is the first mission dedicated to search for transits of exoplanets using ultrahigh precision photometry on bright stars already known to host planets. As a follow-up mission, CHEOPS is mainly dedicated to improving, whenever possible, existing radii measurements or provide first accurate measurements for a subset of those planets for which the mass has already been estimated from ground-based spectroscopic surveys. The expected photometric precision will also allow CHEOPS to go beyond measuring only transits and to follow phase curves or to search for exo-moons, for example. Finally, by unveiling transiting exoplanets with high potential for in-depth characterisation, CHEOPS will also provide prime targets for future instruments suited to the spectroscopic characterisation of exoplanetary atmospheres. To reach its science objectives, requirements on the photometric precision and stability have been derived for stars with magnitudes ranging from 6 to 12 in the V band. In particular, CHEOPS shall be able to detect Earth-size planets transiting G5 dwarf stars (stellar radius of 0.9R) in the magnitude range 6 ≤ V ≤ 9 by achieving a photometric precision of 20 ppm in 6 hours of integration time. In the case of K-type stars (stellar radius of 0.7R) of magnitude in the range 9 ≤ V ≤ 12, CHEOPS shall be able to detect transiting Neptune-size planets achieving a photometric precision of 85 ppm in 3 hours of integration time. This precision has to be maintained over continuous periods of observation for up to 48 hours. This precision and stability will be achieved by using a single, frame-transfer, back-illuminated CCD detector at the focal plane assembly of a 33.5 cm diameter, on-axis Ritchey-Chrétien telescope. The nearly 275 kg spacecraft is nadir-locked, with a pointing accuracy of about 1 arcsec rms, and will allow for at least 1 Gbit/day downlink. The sun-synchronous dusk-dawn orbit at 700 km altitude enables having the Sun permanently on the backside of the spacecraft thus minimising Earth stray light. A mission duration of 3.5 years in orbit is foreseen to enable the execution of the science programme. During this period, 20% of the observing time is available to the wider community through yearly ESA call for proposals, as well as through discretionary time approved by ESA’s Director of Science. At the time of this writing, CHEOPS commissioning has been completed and CHEOPS has been shown to fulfill all its requirements. The mission has now started the execution of its science programme., In Portugal, this work was supported by FCT - Fundação para a Ciência e a Tecnologia through national funds and by FEDER through COMPETE2020 - Programa Operacional Competitividade e Internacionalização by these grants: UID/FIS/04434/2019; UIDB/04434/2020; UIDP/04434/2020; PTDC/FIS-AST/32113/2017 & POCI-01-0145-FEDER-032113; PTDC/FIS-AST/28953/2017 & POCI-01-0145-FEDER-028953; PTDC/FIS-AST/28987/2017 & POCI-01-0145-FEDER-028987. S.C.C.B. and S.G.S. acknowledge support from FCT through FCT contracts nr. IF/01312/2014/CP1215/CT0004, IF/00028/2014/CP1215/CT0002. O.D.S.D. is supported in the form of work contract (DL 57/2016/CP1364/CT0004) funded by national funds through Fundação para a Ciência e Tecnologia (FCT). We also acknowledge support from the Spanish Ministry of Science and Innovation and the European Regional Development Fund through grants ESP2016-80435-C2-1-R, ESP2016-80435-C2-2-R, PGC2018-098153-B-C31, PGC2018-098153-B-C33, ESP2017-87676-C5-1-R, and MDM-2017-0737 Unidad de Excelencia María de Maeztu- Centro de Astrobiología (INTA-CSIC), as well as the support of the Generalitat de Catalunya/CERCA programme. The MOC activities have been supported by the ESA contract No. 4000124370. Finally, XB, SC, DG, MF and JL acknowledge their role as ESA-appointed CHEOPS science team members.
Published: 2021

24. Lieux de mémoire sonore

Author: Laëtitia Atlani-Duault, Luis Velasco-Pufleau, Universität Bern [Bern], Centre population et développement (CEPED - UMR_D 196), Institut de Recherche pour le Développement (IRD)-Université de Paris (UP), Universität Bern [Bern] (UNIBE), and Institut de Recherche pour le Développement (IRD)-Université Paris Cité (UPCité)
Subjects: 060106 history of social sciences, mémoire sonore, son, sound, Vanuatu, 050602 political science & public administration, 0601 history and archaeology, music, Moyen-Orient, lieux de mémoire, musique et migration, musique, Suisse, [SHS.MUSIQ]Humanities and Social Sciences/Musicology and performing arts, music and migration, 05 social sciences, organized violence, Allemagne, Syrie, Liban, 06 humanities and the arts, [SHS.ANTHRO-SE]Humanities and Social Sciences/Social Anthropology and ethnology, 16. Peace & justice, violence organisée, Venezuela, [SHS.SCIPO]Humanities and Social Sciences/Political science, 0506 political science, sonic sites of memory, sonic lieux de mémoire, silence, Viet Nam, sound memory, France, [SHS.HIST]Humanities and Social Sciences/History
Abstract: International audience; In this introduction we argue that sonic experiences in contexts of organized violence can be understood as lieux de mémoire (sites of memory). Exploring how these sonic sites are indissociable from the individual and collective experience of places, we show how they form networks of relationships within which the memory of silences and sounds is constructed and actualized. We also argue that these sonic lieux de mémoire can be seen from two perspectives, representing the dark and bright sides of the same phenomenon. On one hand, sound, music and silence are used as weapons in organized violence, for example in detention facilities or during wars or political conflicts. On the other hand, they constitute symbolic resources, positive tools that contribute to the (re)construction of subjectivities and thus can serve as tools for survival and resistance. In both cases, sound and musical practices are essential facets of what makes us human.; Dans cette introduction nous affirmons que les expériences sonores en contexte de violence organisée peuvent être comprises comme des « lieux de mémoire sonore ». Indissociables de l’expérience individuelle et collective des lieux, ils constituent des réseaux de relations non prédéterminées, dans lesquels la mémoire des silences et des sons se construit et s’actualise. Nous soutenons aussi que les lieux de mémoire sonore peuvent être appréhendés sous une double perspective, à la fois la face noire et la face lumineuse d’un même phénomène. D’une part, le son, la musique et le silence sont utilisés comme des armes en contexte de violence organisée, que cela soit par exemple dans certains lieux de détention ou en situation de guerre ou de conflit politique. D’autre part, ils constituent des ressources symboliques qui contribuent à la (re)construction de subjectivités, notamment dans des situations faisant suite à des expériences d’exil forcé et de violence organisée. Dans tous les cas, les pratiques sonores et musicales sont des ressources immatérielles constitutives des êtres humains.
Published: 2021

25. Geomorphic response to the Lateglacial-Holocene transition in high Alpine regions (Sanetsch Pass, Swiss Alps)

Author: Serra, Elena, Valla, Pierre, Gribenski, Natacha, Guedes Magrani, Fabio, Carcaillet, Julien, delaloye, Reynald, Grobéty, Bernard, Braillard, Luc, Institut für Geologie [Bern], Universität Bern [Bern], Institut des Sciences de la Terre (ISTerre), Institut national des sciences de l'Univers (INSU - CNRS)-Institut de recherche pour le développement [IRD] : UR219-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Gustave Eiffel-Université Grenoble Alpes (UGA), UNIVERSITY OF FRIBOURG DEPARTMENT OF GEOSCIENCES GEOGRAPHY CHE, Partenaires IRSTEA, Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA), Universität Bern [Bern] (UNIBE), and Institut national des sciences de l'Univers (INSU - CNRS)-Institut de recherche pour le développement [IRD] : UR219-Université Grenoble Alpes (UGA)-Université Gustave Eiffel-Centre National de la Recherche Scientifique (CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])
Subjects: [SDE]Environmental Sciences
Abstract: Several palaeoclimatic archives have documented the pronounced climatic and environmental change associated with the Lateglacial–Holocene transition in the European Alps. However, the geomorphic response to this major environmental transition has only been punctually investigated. In this study, we propose a detailed reconstruction of post‐Last Glacial Maximum palaeoenvironmental conditions and geomorphic connectivity in the Sanetsch Pass area (2252 m a.s.l., western Swiss Alps) based on a multi‐method approach combining geomorphological and sedimentological field investigations with quantitative sedimentology and geochronology. Samples for sediment characterization (grain size, micromorphology and X‐ray diffraction) and geochronology (optically stimulated luminescence and 10Be surface exposure dating) were collected from three representative landforms of the study area: a high‐elevation silty deposit covered by patterned ground, an alluvial fan, and a hummocky moraine covered by rockfall deposits. Our results reveal the geomorphic history of the three deposits and their connectivity through sediment cascade. These results highlight the development of rapid and most probably transient landscape changes in high Alpine regions during the Lateglacial–Holocene transition, with an increase in sediment flux and the establishment of paraglacial and periglacial geomorphic processes.
Published: 2021

26. Visualizing the evolution of evidence: Cumulative network meta‐analyses of new generation antidepressants in the last 40 years

Author: Yusuke Ogawa, Anna Chaimani, Georgia Salanti, Toshi A. Furukawa, Yuki Kataoka, Yan Luo, Andrea Cipriani, Chaimani, Anna, Kyoto University, Centre de Recherche Épidémiologie et Statistique Sorbonne Paris Cité (CRESS (U1153 / UMR_A_1125 / UMR_S_1153)), Conservatoire National des Arts et Métiers [CNAM] (CNAM), HESAM Université - Communauté d'universités et d'établissements Hautes écoles Sorbonne Arts et métiers université (HESAM)-HESAM Université - Communauté d'universités et d'établissements Hautes écoles Sorbonne Arts et métiers université (HESAM)-Université Sorbonne Paris Cité (USPC)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université Paris Cité (UPCité)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Amagasaki General Medical Center [Hyogo, Japan] (Hospital Care Research Unit), University of Oxford, Institute of Social and Preventive Medicine [Bern] (ISPM), Universität Bern [Bern] (UNIBE), Kyoto University [Kyoto], Conservatoire National des Arts et Métiers [CNAM] (CNAM)-Université Sorbonne Paris Cité (USPC)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université de Paris (UP)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), University of Oxford [Oxford], and Universität Bern [Bern]
Subjects: Treatment response, Computer science, confidence in the evidence, [SDV]Life Sciences [q-bio], Psychological intervention, 610 Medicine & health, 01 natural sciences, History, 21st Century, Education, law.invention, 010104 statistics & probability, 03 medical and health sciences, 0302 clinical medicine, Randomized controlled trial, 360 Social problems & social services, law, Special Issue Paper, network meta‐analysis, Humans, 030212 general & internal medicine, 0101 mathematics, network meta-analysis, visualization, Depressive Disorder, Major, Actuarial science, Evidence-Based Medicine, Special Issue Papers, evidence evolution, Data Visualization, shiny, Odds ratio, History, 20th Century, Confidence interval, Antidepressive Agents, 3. Good health, Discontinuation, [SDV] Life Sciences [q-bio], Network Meta-Analyses, Meta-analysis, Data Interpretation, Statistical, Software
Abstract: It is often challenging to present the available evidence in a timely and comprehensible manner. We aimed to visualize the evolution of evidence about antidepressants for depression by conducting cumulative network meta-analyses (NMAs) and to examine whether it could have helped the selection of optimal drugs. We built a Shiny web application that performs and presents cumulative NMAs based on R netmeta. We used a comprehensive dataset of double-blind randomized controlled trials of 21 antidepressants in the acute treatment of major depression. The primary outcomes were efficacy (treatment response) and acceptability (all-cause discontinuation), and treatment effects were summarized via odds ratios. We evaluated the confidence in evidence using the CINeMA (Confidence in Network Meta-Analysis) framework for a series of consecutive NMAs. Users can change several conditions for the analysis, such as the period of synthesis, among the others. We present the league tables and two-dimensional plots that combine efficacy, acceptability and level of confidence in the evidence together, for NMAs conducted in 1990, 1995, 2000, 2005, 2010, and 2016. They reveal that through the past four decades, newly approved drugs often showed initially exaggerated results, which tended to diminish and stabilize after approximately a decade. Over the years, the drugs with relative superiority changed dramatically; but as the evidence network grew larger and better connected, the overall confidence improved. The Shiny app visualizes how evidence evolved over years, emphasizing the need for a careful interpretation of relative effects between drugs, especially for the potentially amplified performance of newly approved drugs. HIGHLIGHTS: Network meta-analysis is considered to be a proper way of demonstrating the available evidence, since it allows comparisons between multiple interventions, and has been proved to be statistically powerful. It is challenging to present the voluminous results of NMA in an efficient and comprehendible manner. Evidence evolution based on the relatively new method NMA has not been investigated yet. The results of NMA should not only include the effects but also the confidence in the evidence, which can help interpret the findings appropriately. Effective use of rapidly developing statistical analysis and presentation tools such as Shiny package in R, may facilitate and simplify the visualization of NMA output. We should stay conservative towards new drugs, as their performance was often shown to be exaggerated initially, and it took time to become stable.
Published: 2021

27. Music, Noise and Conflict: Sociotechnical Imaginaries, Acoustic Agency and Ontological Assumptions about Sound

Author: Luis Velasco-Pufleau, Universität Bern [Bern], McGill University = Université McGill [Montréal, Canada], Marie Skłodowska-Curie Actions, European Project: 101027828,ONTOMUSIC, Universität Bern [Bern] (UNIBE), and Schulich School of Music [Montréal]
Subjects: noise, Sociotechnical system, 060106 history of social sciences, Acoustics, conflict, 300 Social sciences, sociology & anthropology, 780 Music, 060404 music, sound, Agency (sociology), 0601 history and archaeology, music, Sociology, Sound (geography), geography, geography.geographical_feature_category, ontological assumptions, [SHS.MUSIQ]Humanities and Social Sciences/Musicology and performing arts, sonic archives, media, [SHS.PHIL]Humanities and Social Sciences/Philosophy, 06 humanities and the arts, [SHS.SCIPO]Humanities and Social Sciences/Political science, Noise, affect, silence, politics, sociotechnical imaginaries, aural experiences, [SHS.HIST]Humanities and Social Sciences/History, 0604 arts, 900 History
Abstract: International audience; How are sociotechnical imaginaries and ontological assumptions about sound related to affect and conflict spaces? What do sociotechnical imaginaries tell us about social and individual control of sonic environments? Why is it important to think about ontological assumptions of sound when recovering aural experiences of the past in archives? The three books under consideration in this review article address these questions in different ways. They explore the use of media devices to produce affect and social relations, the role of categories of music and noise in the control of urban spaces, and the politics of archival sounds and silence.
Published: 2021

28. The Early Bronze Age dendrochronology of Sovjan (Albania): A first tree-ring sequence of the 24th – 22nd c. BC for the southwestern Balkans

Author: Cécile Oberweiler, Ariane Ballmer, Gilles Touchais, Petrika Lera, Maja Gori, Albert Hafner, Andrej Maczkowski, Sönke Szidat, Matthias Bolliger, Archéologie et Philologie d'Orient et d'Occident (AOROC), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École pratique des hautes études (EPHE), Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Consiglio Nazionale delle Ricerche (CNR), Université Fan S. Noli de Korçë, Institut archéologique de Tirana, Archéologies et Sciences de l'Antiquité (ArScAn), Centre National de la Recherche Scientifique (CNRS)-Ministère de la Culture et de la Communication (MCC)-Université Paris Nanterre (UPN)-Université Paris 1 Panthéon-Sorbonne (UP1), Oeschger Centre for Climate Change Research (OCCR), University of Bern, Universität Bern [Bern], Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-École pratique des hautes études (EPHE), Université Paris sciences et lettres (PSL), Université Paris 1 Panthéon-Sorbonne (UP1)-Université Paris Nanterre (UPN)-Ministère de la Culture et de la Communication (MCC)-Centre National de la Recherche Scientifique (CNRS), École pratique des hautes études (EPHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Département des Sciences de l'Antiquité - ENS Paris (DSA ENS-PSL), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS-PSL), Université Paris 1 Panthéon-Sorbonne (UP1)-Université Paris 8 Vincennes-Saint-Denis (UP8)-Université Paris Nanterre (UPN)-Ministère de la Culture et de la Communication (MCC)-Institut national de recherches archéologiques préventives (Inrap)-Centre National de la Recherche Scientifique (CNRS), Protohistoire égéenne (ProtoEgéenne), Université Paris 1 Panthéon-Sorbonne (UP1)-Université Paris 8 Vincennes-Saint-Denis (UP8)-Université Paris Nanterre (UPN)-Ministère de la Culture et de la Communication (MCC)-Institut national de recherches archéologiques préventives (Inrap)-Centre National de la Recherche Scientifique (CNRS)-Université Paris 1 Panthéon-Sorbonne (UP1)-Université Paris 8 Vincennes-Saint-Denis (UP8)-Université Paris Nanterre (UPN)-Ministère de la Culture et de la Communication (MCC)-Institut national de recherches archéologiques préventives (Inrap)-Centre National de la Recherche Scientifique (CNRS), and Universität Bern [Bern] (UNIBE)
Subjects: 0106 biological sciences, 930 History of ancient world (to ca. 499), Sovjan -- Albania, 010504 meteorology & atmospheric sciences, [SHS.ARCHEO]Humanities and Social Sciences/Archaeology and Prehistory, Dendrochronological dating, Plant Science, 01 natural sciences, [SHS]Humanities and Social Sciences, Prehistory, Sequence (geology), Bronze Age, 540 Chemistry, Dendrochronology, Early Bronze Age, Sequence stratigraphy, ComputingMilieux_MISCELLANEOUS, 0105 earth and related environmental sciences, Ecology, Trackway, Archaeology, Iron Age, 570 Life sciences, biology, 900 History, 010606 plant biology & botany, Chronology
Abstract: The archaeological site of Sovjan is situated on the edge of the Korce Basin, southeastern Albania. Its remarkably long and well investigated stratigraphic sequence, spanning from the Neolithic till the Iron Age, makes it an important type- and reference-site for the whole region. At different periods of prehistory it was located on the shores of the former Lake Maliq that once filled the Korce Basin, but was definitely drained in the 1940′s. These permanent wetland conditions on the site allowed for a high degree of preservation of organic material, especially wood. Based on the current knowledge, level 8 of Sovjan contains the best-preserved wooden material of all the Early Bronze Age sites in the Balkans. Through the combination of dendrochronology and Bayesian modelling, i.e. wiggle-matching, a floating 269-years long tree-ring chronology was constructed, with an absolute end-date range falling between 2158 and 2142 cal BC (2σ). It was possible to establish that the dwellings and the trackway associated with the last occupation phase of level 8 are contemporaneous. Additionally, with the help of the new dendrochronological data and based on previously published charcoal dates, the absolute chronology of the subsequent level 7 is being narrowed-down to a range from the mid-22nd to mid-20th c. cal BC (2σ). The Early Bronze Age layers of the archaeological site of Sovjan, which are particularly pertinent for the 3rd millennium chronology of the southwestern Balkans, can now be dated with high precision for the first time and hence offer a major chronological reference point in the region.
Published: 2021
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29. New constraints on the chemical composition and outgassing of 67P/Churyumov-Gerasimenko

Author: O. Pinzón-Rodríguez, Raphael Marschall, Nicolas Thomas, O. Mousis, Clémence Herny, Ian Wright, Martin Rubin, Physikalisches Institut [Bern], Universität Bern [Bern] (UNIBE), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Southwest Research Institute [Boulder] (SwRI), Universität Bern [Bern], and Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES)
Subjects: 010504 meteorology & atmospheric sciences, Comet composition and internal structure, 520 Astronomy, Comet, Northern Hemisphere, Astronomy and Astrophysics, Astrophysics, 620 Engineering, 01 natural sciences, Mantle (geology), Thermal modelling of cometary nucleus ROSINA/DFMS data, Latitude, Outgassing, 13. Climate action, Space and Planetary Science, Comet 67P/Churyumov-Gerasimenko, [SDU]Sciences of the Universe [physics], Volatiles outgassing, 0103 physical sciences, Sublimation (phase transition), 010303 astronomy & astrophysics, Chemical composition, Southern Hemisphere, Geology, 0105 earth and related environmental sciences
Abstract: International audience; Strong heterogeneities in the composition of the volatile species have been detected in the coma of comet 67P/Churyumov-Gerasimenko (67P/C-G) by the ROSINA instrument onboard the ESA’s Rosetta spacecraft. However, it is not clear if these heterogeneities are indicative of heterogeneities in the near-surface nucleus composition or if the coma composition is mainly insolation-driven. In order to clarify the link between the composition of the nucleus and the composition of the coma we have performed numerical simulations and compare our results with measurements acquired by ROSINA/DFMS for three major volatile species namely, H2O, CO2, and CO. We use a previously published thermo-physical numerical model designed to study cometary nucleus evolution, including volatile outgassing and internal stratigraphy, as the comet orbits the Sun. The model follows schemes used for much of the past three decades to model cometary outgassing. Our results match well the experimental volatiles density measurements of ROSINA/DFMS for most of the Rosetta mission. They suggest that the outgassing pattern is mainly insolation-driven and the variations are caused by the tilt of rotation axis and eccentricity of the nucleus. The nucleus shows to 1st order a homogeneous composition and therefore we can provide constraints on the bulk volatiles composition of 67P/C-G nucleus which is dominated by H2O (91.4% ± 4.5%), then CO2 (6.7% ± 3.5%) and CO in small amount (1.9% ± 1.2%). However, in details, a dichotomy in composition between the northern and southern hemispheres of the comet is revealed. A CO/CO2 bulk composition ratio of about 0.6 ± 0.1 is required to reproduce the measurements from the northern hemisphere and about 0.2 ± 0.1 for the southern hemisphere. To match the data, the thermal properties of the nucleus surface must be modified by adding a thin desiccated dust mantle (~5 mm) for northern latitudes while this appears not to be necessary for southern latitudes. This may be related to the observed dichotomy in putative airfall deposits. We suspect that, because of thermal inertia, seasonally non-illuminated areas continue to outgas and influence the ROSINA measurements. This effect cannot be reproduced with the model. Therefore during some periods of the mission, the fits are not ideal. Finally, the outgassing of the different ices leads to a layered internal structure defined by the sublimation front of each ice and formation of harder layers close to the surface due to sublimation/condensation processes. However, the thermo-physical model overestimates the absolute volatiles production (mainly in the southern hemisphere) leading to an overestimation of the erosion rates. Further investigations will be performed to improve the thermo-physical model and the sensitivity analysis.
Published: 2021
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30. Clues from ab initio calculations on titanium isotopic fractionation in tholeiitic and calc-alkaline magma series

Author: Timo Hopp, Nicolas Dauphas, Hao Zeng, N. X. Nie, S. M. Aarons, Nicolas D. Greber, Aleisha C. Johnson, Marc Blanchard, Department of the Geophysical Sciences, University of Chicago, Scripps Institution of Oceanography (SIO - UC San Diego), University of California [San Diego] (UC San Diego), University of California (UC)-University of California (UC), Géosciences Environnement Toulouse (GET), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Carnegie Institution for Science, Universität Bern [Bern] (UNIBE), Scripps Institution of Oceanography (SIO), University of California-University of California, Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD), Carnegie Institution for Science [Washington], and Universität Bern [Bern]
Subjects: Atmospheric Science, 010504 meteorology & atmospheric sciences, Analytical chemistry, Fractionation, engineering.material, 010502 geochemistry & geophysics, 01 natural sciences, chemistry.chemical_compound, Isotope fractionation, Geochemistry and Petrology, [SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistry, 550 Earth sciences & geology, Titanite, titanium, isotopes, 0105 earth and related environmental sciences, fractional crystallization, Diopside, Fractional crystallization (geology), Chemistry, Calc-alkaline magma series, ab initio, Silicate, Space and Planetary Science, visual_art, engineering, visual_art.visual_art_medium, isotopic fractionation, Igneous differentiation, [SDU.STU.MI]Sciences of the Universe [physics]/Earth Sciences/Mineralogy
Abstract: International audience; Magmatic differentiation produces positive correlations between δ49Ti and SiO2. The equilibrium Ti isotope fractionation factors of Ti-bearing minerals are essential for understanding the mechanisms driving this isotopic fractionation. We present ab initio-derived mean force constants of Ti-bearing minerals (barium orthotitanate, potassium titanium oxide, fresnoite, diopside, geikielite, karrooite, titanite, pseudobrookite, anatase, and titanium oxide) based on density functional theory (DFT) to calculate equilibrium isotopic fractionation factors. We find that the main driver for Ti isotopic fractionation is its coordination, with four-, five-, and sixfold-coordinated Ti characterized by mean force constants of 547, 462, and 310 N/m, respectively. The coordination number of Ti in silicate melts is thought to be lower than in minerals, driving magmas toward higher δ49Ti values by fractional crystallization. The mineral-melt fractionation factors allow modeling of the observed Ti isotope trends in tholeiitic and calc-alkaline rocks. Our model results indicate that to first order, the steeper δ49Ti trend observed in tholeiitic versus calc-alkaline magmas is most likely due to enhanced removal of Ti into sequestered minerals at low SiO2 concentration in tholeiitic series compared to calc-alkaline series. The δ49Ti–SiO2 differentiation trends, however, depend on Ti coordination in the melt and the strengths of Ti bonds in diverse Fe- and Ti-oxides, which are still uncertain. Our results show that Ti isotopes can be used to reconstruct the crystallization history and identify the magmatic series parentage of magmas that otherwise lack context, but further work is needed to identify the drivers behind Ti isotopic fractionation in igneous rocks.
Published: 2021

31. Why do large-scale agricultural investments induce different socio-economic, food security, and environmental impacts? Evidence from Kenya, Madagascar, and Mozambique

Author: Oberlack, Christoph, Giger, Markus, Anseeuw, Ward, Adelle, Camilla, Bourblanc, Magalie, Burnod, Perrine, Eckert, Sandra, Fitawek, Wegayehu, Fouilleux, Eve, Hendriks, Sheryl L., Kiteme, Boniface, Masola, Livhuwani, Mawoko, Zaka Diana, Mercandalli, Sara, Reys, Aur��lien, da Silva, Maya, van der Laan, Michael, Zaehringer, Julie G., Messerli, Peter, Centre for Development and Environment [Bern] (CDE), Universität Bern [Bern], Institute of Geography [Bern], University of Bern, Acteurs, Ressources et Territoires dans le Développement (UMR ART-Dev), Centre de Coopération Internationale en Recherche Agronomique pour le Développement (Cirad)-Université Paul-Valéry - Montpellier 3 (UPVM)-Université de Perpignan Via Domitia (UPVD)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Département Environnements et Sociétés (Cirad-ES), Centre de Coopération Internationale en Recherche Agronomique pour le Développement (Cirad), International Land Coalition (ILC), University of Pretoria [South Africa], Gestion de l'Eau, Acteurs, Usages (UMR G-EAU), Centre de Coopération Internationale en Recherche Agronomique pour le Développement (Cirad)-Institut de Recherche pour le Développement (IRD)-AgroParisTech-Institut national d’études supérieures agronomiques de Montpellier (Montpellier SupAgro), Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro)-Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Territoires, Environnement, Télédétection et Information Spatiale (UMR TETIS), Centre de Coopération Internationale en Recherche Agronomique pour le Développement (Cirad)-AgroParisTech-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Malagasy Land Observatory, Montpellier Interdisciplinary center on Sustainable Agri-food systems (Social and nutritional sciences) (UMR MoISA), Centre de Coopération Internationale en Recherche Agronomique pour le Développement (Cirad)-Institut de Recherche pour le Développement (IRD)-Centre International de Hautes Etudes Agronomiques Méditerranéennes - Institut Agronomique Méditerranéen de Montpellier (CIHEAM-IAMM), Centre International de Hautes Études Agronomiques Méditerranéennes (CIHEAM)-Centre International de Hautes Études Agronomiques Méditerranéennes (CIHEAM)-Institut national d’études supérieures agronomiques de Montpellier (Montpellier SupAgro), Laboratoire Interdisciplinaire Sciences, Innovations, Sociétés (LISIS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Gustave Eiffel, Centre for Training and Integrated Research in ASAL Development (CETRAD), Centre de Coopération Internationale en Recherche Agronomique pour le Développement (Cirad)-Institut de Recherche pour le Développement (IRD)-AgroParisTech-Institut national d’études supérieures agronomiques de Montpellier (Montpellier SupAgro)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Centre International de Hautes Études Agronomiques Méditerranéennes (CIHEAM)-Centre International de Hautes Études Agronomiques Méditerranéennes (CIHEAM)-Institut national d’études supérieures agronomiques de Montpellier (Montpellier SupAgro)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Centre National de la Recherche Scientifique (CNRS)-Centre de Coopération Internationale en Recherche Agronomique pour le Développement (Cirad)-Université de Montpellier (UM)-Université de Perpignan Via Domitia (UPVD)-Université Paul-Valéry - Montpellier 3 (UPVM), Marchés, Organisations, Institutions et Stratégies d'Acteurs (UMR MOISA), Institut national d’études supérieures agronomiques de Montpellier (Montpellier SupAgro)-Centre International de Hautes Etudes Agronomiques Méditerranéennes - Institut Agronomique Méditerranéen de Montpellier (CIHEAM-IAMM), Centre International de Hautes Études Agronomiques Méditerranéennes (CIHEAM)-Centre International de Hautes Études Agronomiques Méditerranéennes (CIHEAM)-Institut National de la Recherche Agronomique (INRA)-Centre de Coopération Internationale en Recherche Agronomique pour le Développement (Cirad)-Centre international d'études supérieures en sciences agronomiques (Montpellier SupAgro), Universität Bern [Bern] (UNIBE), Centre de Coopération Internationale en Recherche Agronomique pour le Développement (Cirad)-Institut de Recherche pour le Développement (IRD)-AgroParisTech-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut Agro - Montpellier SupAgro, Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro)-Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro), and Centre International de Hautes Études Agronomiques Méditerranéennes (CIHEAM)-Centre International de Hautes Études Agronomiques Méditerranéennes (CIHEAM)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut Agro - Montpellier SupAgro
Subjects: F08 - Systèmes et modes de culture, changement dans l'usage des terrres, Environment, E13 - Investissements, financement et crédit, Business models, [SHS]Humanities and Social Sciences, enquêtes auprès des ménages, impacts socio-économiques, Land use change, Livelihoods, E10 - Économie et politique agricoles, Utilisation des terres, Governance, Stratégies de développement rural, Économie agricole, Impact sur l'environnement, [SDV.SA.AEP]Life Sciences [q-bio]/Agricultural sciences/Agriculture, economy and politics, Food security, [SHS.ECO]Humanities and Social Sciences/Economics and Finance, [SDE.ES]Environmental Sciences/Environmental and Society, sécurité alimentaire, Investissement, Agricultural investments
Abstract: International audience; Large-scale agricultural investments (LAIs) transform land use systems worldwide. There is, however, limited understanding about how the common global drivers of land use change induce different forms of agricultural investment and produce different impacts on the ground. This article provides a cross-country comparative analysis of how differences in business models, land use changes, and governance systems explain differences in socio-economic, food security, and environmental impacts of LAIs in Kenya, Madagascar, and Mozambique. It brings together results on these aspects generated in the AFGROLAND project that collected data in a multi-method approach via household surveys, business model surveys, semi-structured household interviews, life-cycle assessments of farm production, analysis of remote-sensing data, key informant interviews, and document analysis. For the present project synthesis, we combined a collaborative expert workshop with a comparative analysis of 16 LAIs. The results show that the LAIs follow four distinctive impact patterns, ranging from widespread adverse impacts to moderate impacts. Results demonstrate how the following conditions influence how the global drivers of land use change translate into different LAIs and different impacts on the ground: labor intensity, prior land use, utilization of land, farm size, type of production, experience in local agriculture, land tenure security, accountability of state and local elites, the mobilization capacity of civil society, expansion of resource frontiers, agricultural intensification, and indirect land use change. The results indicate that commercial agriculture can be a component in sustainable development strategies under certain conditions, but that these strategies will fail without substantial, sustained increases in the economic viability and inclusiveness of smallholder agriculture, land tenure security, agro-ecological land management, and support for broader patterns of endogenous agrarian transformation.
Published: 2021

32. Compound climate events and extremes in the mid-latitudes: dynamics, simulation and statistical characterisation

Author: Pascal Yiou, Colin Raymond, Paolo De Luca, Kai Kornhuber, Olivia Martius, Dim Coumou, Davide Faranda, Emanuele Bevacqua, Gabriele Messori, Kunhui Ye, Rodrigo Caballero, Jakob Zscheischler, Flavio Maria Emanuele Pons, Uppsala University, University of Reading (UOR), Stockholm University, Vrije Universiteit Amsterdam [Amsterdam] (VU), Royal Netherlands Meteorological Institute (KNMI), Laboratoire de Météorologie Dynamique (UMR 8539) (LMD), Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-École des Ponts ParisTech (ENPC)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Département des Géosciences - ENS Paris, École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), London Mathematical Laboratory, Laboratoire des Sciences du Climat et de l'Environnement [Gif-sur-Yvette] (LSCE), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ), Extrèmes : Statistiques, Impacts et Régionalisation (ESTIMR), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ), Columbia University [New York], Universität Bern [Bern], Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Helmholtz Zentrum für Umweltforschung = Helmholtz Centre for Environmental Research (UFZ), Water and Climate Risk, Earth and Climate, École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS-PSL), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), and Universität Bern [Bern] (UNIBE)
Subjects: Climate events, Atmospheric Science, Climate Research, 010504 meteorology & atmospheric sciences, Atmospheric circulation, 530 Physics, 0211 other engineering and technologies, 02 engineering and technology, [SDU.STU.ME]Sciences of the Universe [physics]/Earth Sciences/Meteorology, 01 natural sciences, Klimatforskning, Statistical techniques, Extreme events, 910 Geography & travel, ComputingMilieux_MISCELLANEOUS, 0105 earth and related environmental sciences, 021110 strategic, defence & security studies, Characterization (materials science), 13. Climate action, [SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology, Climatology, Middle latitudes, Environmental science
Abstract: The workshop, conducted virtually due to travel restrictions related to COVID-19, gathered scientists from six countries and focused on the mechanistic understanding, statistical characterization, and modeling of societally relevant compound climate events and extremes in the midlatitudes. These ranged from co-occurring hot–humid or wet–windy extremes, to spatially compounding wet and dry extremes, to temporally compounding hot–wet events and more. The aim was to bring together selected experts studying a diverse range of compound climate events and extremes to present their ongoing work and outline challenges and future developments in this societally relevant field of research.
Published: 2021

33. Towards a compound-event-oriented climate model evaluation: a decomposition of the underlying biases in multivariate fire and heat stress hazards

Author: Jakob Zscheischler, Roberto Villalobos-Herrera, Bilyana Mircheva, Minh Ha, Emanuele Bevacqua, Laura Crocetti, Graeme Auld, Carlo De Michele, Andreia F. S. Ribeiro, School of Engineering [Newcastle], Newcastle University [Newcastle], Escuela de Ingeniería Civil [Costa Rica], Universidad de Costa Rica (UCR), Department of Meteorology [Reading], University of Reading (UOR), Instituto Dom Luiz, Universidade de Lisboa (ULISBOA), School of Mathematics - University of Edinburgh, University of Edinburgh, Department of Geodesy and Geoinformation [Wien], Vienna University of Technology (TU Wien), Institute of Geodesy and Photogrammetry [Zürich] (IGP), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Department of Meteorology and Geophysics [Sofia], Sofia University 'St. Kliment Ohridski', SPACE - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Climate and Environmental Physics [Bern] (CEP), Physikalisches Institut [Bern], Universität Bern [Bern]-Universität Bern [Bern], Oeschger Centre for Climate Change Research (OCCR), University of Bern, Helmholtz Zentrum für Umweltforschung = Helmholtz Centre for Environmental Research (UFZ), Dipartimento di Ingegneria Civile e Ambientale (DICA), and Politecnico di Milano [Milan] (POLIMI)
Subjects: Multivariate statistics, 010504 meteorology & atmospheric sciences, 530 Physics, Wet-bulb globe temperature, 0208 environmental biotechnology, 02 engineering and technology, Environmental technology. Sanitary engineering, 01 natural sciences, Geography. Anthropology. Recreation, Econometrics, GE1-350, TD1-1066, 0105 earth and related environmental sciences, Event (probability theory), QE1-996.5, Univariate, Geology, Hazard, 020801 environmental engineering, Heat stress, Environmental sciences, [SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatology, 13. Climate action, General Earth and Planetary Sciences, Environmental science, Common spatial pattern, Climate model
Abstract: Climate models' outputs are affected by biases that need to be detected and adjusted to model climate impacts. Many climate hazards and climate-related impacts are associated with the interaction between multiple drivers, i.e. by compound events. So far climate model biases are typically assessed based on the hazard of interest, and it is unclear how much a potential bias in the dependence of the hazard drivers contributes to the overall bias and how the biases in the drivers interact. Here, based on copula theory, we develop a multivariate bias-assessment framework, which allows for disentangling the biases in hazard indicators in terms of the underlying univariate drivers and their statistical dependence. Based on this framework, we dissect biases in fire and heat stress hazards in a suite of global climate models by considering two simplified hazard indicators: the wet-bulb globe temperature (WBGT) and the Chandler burning index (CBI). Both indices solely rely on temperature and relative humidity. The spatial pattern of the hazard indicators is well represented by climate models. However, substantial biases exist in the representation of extreme conditions, especially in the CBI (spatial average of absolute bias: 21 ∘C) due to the biases driven by relative humidity (20 ∘C). Biases in WBGT (1.1 ∘C) are small compared to the biases driven by temperature (1.9 ∘C) and relative humidity (1.4 ∘C), as the two biases compensate for each other. In many regions, also biases related to the statistical dependence (0.85 ∘C) are important for WBGT, which indicates that well-designed physically based multivariate bias adjustment procedures should be considered for hazards and impacts that depend on multiple drivers. The proposed compound-event-oriented evaluation of climate model biases is easily applicable to other hazard types. Furthermore, it can contribute to improved present and future risk assessments through increasing our understanding of the biases' sources in the simulation of climate impacts.
Published: 2021

34. On the origin & thermal stability of Arrokoth's and Pluto's ices

Author: Marc Neveu, Harold A. Weaver, Mohamed Ramy El-Maarry, J. M. Parker, John R. Spencer, William B. McKinnon, Scott A. Sandford, Alissa M. Earle, Orkan M. Umurhan, Mihaly Horanyi, Ralph L. McNutt, G. R. Gladstone, Andrew F. Cheng, Catherine B. Olkin, R. P. Binzel, Y. J. Pendleton, Carey M. Lisse, Olivier Mousis, William M. Grundy, Jj Kavelaars, J. T. Keane, N. Dello-Russo, Wladimir Lyra, Jordan K. Steckloff, S. A. Stern, Ivan Linscott, Bernard Schmitt, H. A. Elliott, Leslie A. Young, Dale P. Cruikshank, Daniel T. Britt, B. L. Lewis, J. M. Moore, Johns Hopkins University Applied Physics Laboratory [Laurel, MD] (APL), Southwest Research Institute [Boulder] (SwRI), NASA Ames Research Center (ARC), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA), Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Southwest Research Institute [San Antonio] (SwRI), Department of Earth, Atmospheric and Planetary Sciences [MIT, Cambridge] (EAPS), Massachusetts Institute of Technology (MIT), Laboratory for Atmospheric and Space Physics [Boulder] (LASP), University of Colorado [Boulder], Physikalisches Institut [Bern], Universität Bern [Bern], Washington University in Saint Louis (WUSTL), Lowell Observatory [Flagstaff], Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Centre National d'Etudes Spatiales (CNES), NASA for financial support of the New Horizons project, Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, and Universität Bern [Bern] (UNIBE)
Subjects: Earth and Planetary Astrophysics (astro-ph.EP), Physics, Solar System, 010504 meteorology & atmospheric sciences, Young stellar object, Comet, [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, 01 natural sciences, Pluto, Outgassing, Stars, Supernova, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, 0103 physical sciences, Trans-Neptunian object, 010303 astronomy & astrophysics, Solar and Stellar Astrophysics (astro-ph.SR), Astrophysics - Earth and Planetary Astrophysics, 0105 earth and related environmental sciences
Abstract: We discuss in a thermodynamic, geologically empirical way the long-term nature of the stable majority ices that could be present in Kuiper Belt Object 2014 MU69 after its 4.6 Gyr residence in the EKB as a cold classical object. Considering the stability versus sublimation into vacuum for the suite of ices commonly found on comets, Centaurs, and KBOs at the average ~40K sunlit surface temperature of MU69 over Myr to Gyr, we find only 3 common ices that are truly refractory: HCN, CH3OH, and H2O (in order of increasing stability). NH3 and H2CO ices are marginally stable and may be removed by any positive temperature excursions in the EKB, as produced every 1e8 - 1e9 yrs by nearby supernovae and passing O/B stars. To date the NH team has reported the presence of abundant CH3OH and evidence for H2O on MU69s surface (Lisse et al. 2017, Grundy et al. 2020). NH3 has been searched for, but not found. We predict that future absorption feature detections will be due to an HCN or poly-H2CO based species. Consideration of the conditions present in the EKB region during the formation era of MU69 lead us to infer that it formed "in the dark", in an optically thick mid-plane, unable to see the nascent, variable, highly luminous Young Stellar Object-TTauri Sun, and that KBOs contain HCN and CH3OH ice phases in addition to the H2O ice phases found in their Short Period comet descendants. Finally, when we apply our ice thermal stability analysis to bodies/populations related to MU69, we find that methanol ice may be ubiquitous in the outer solar system; that if Pluto is not a fully differentiated body, then it must have gained its hypervolatile ices from proto-planetary disk sources in the first few Myr of the solar systems existence; and that hypervolatile rich, highly primordial comet C/2016 R2 was placed onto an Oort Cloud orbit on a similar timescale., Comment: 34 Pages, 5 Figures, 2 SOM Tables
Published: 2021

35. Huff and puff and blow down: invasive plants traits response to strong winds at the Southern Oceanic Islands

Author: Hugo Saiz, Sara Puijalon, Miguel Barrio, Mathilde Bertrand, Clémentine Prouteau, Anne-Kristel Bittebiere, Aurélien Pierre, Charly Ferreira, David Renault, Matteo Tolosano, Universität Bern [Bern], Ecosystèmes, biodiversité, évolution [Rennes] (ECOBIO), Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Rennes (OSUR)-Institut Ecologie et Environnement (INEE), Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES), Institut Universitaire de France (IUF), Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.), Équipe 2 - Écologie Végétale et Zones Humides (EVZH), Laboratoire d'Ecologie des Hydrosystèmes Naturels et Anthropisés (LEHNA), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-École Nationale des Travaux Publics de l'État (ENTPE)-Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-École Nationale des Travaux Publics de l'État (ENTPE)-Centre National de la Recherche Scientifique (CNRS), Équipe 1 - Biodiversité et Adaptation dans les Hydrosystèmes (BAH), Institut Polaire Francais Paul-Emile Victor [IPEV 136], long-term research network on biodiversity in Antarctic and sub-Antarctic ecosystems (Zone Atelier InEE-CNRS Antarctique et Terres Australes), 2019-2020 BiodivERsA joint call for research proposals, under the BiodivClim ERA-Net COFUND programme, ANR French National Research Agency (ANR) [ANR-20-EBI5-0004], ANR-20-EBI5-0004,ASICS,ASsessing and mitigating the effects of climate change and biological Invasions on the spatial redistribution of biodiversity in Cold environmentS(2020), Universität Bern [Bern] (UNIBE), Université de Rennes (UR)-Institut Ecologie et Environnement (INEE), Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Rennes (OSUR), and Université de Rennes (UR)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Centre National de la Recherche Scientifique (CNRS)
Subjects: 0106 biological sciences, environmental filter, Biodiversity, 010603 evolutionary biology, 01 natural sciences, Invasive species, hypervolume, Resource Acquisition Is Initialization, functional traits, intraspecific variability, Ecology, Evolution, Behavior and Systematics, 2. Zero hunger, Ecological niche, Biomass (ecology), Ecology, mechanical stress, food and beverages, Plant community, 15. Life on land, Geography, Habitat, 13. Climate action, Iles Kerguelen, Trait, [SDE.BE]Environmental Sciences/Biodiversity and Ecology, 010606 plant biology & botany
Abstract: Invasions constitute a major driver of biodiversity changes. Insular plant communities are particularly vulnerable to invasions and are relevant models for investigating mechanisms supporting the establishment and spread of introduced plants. Terrestrial flora of sub-Antarctic islands must often thrive in highly windy habitats, thus imposing strong mechanical constraints on individuals. Many alien plants at the sub-Antarctic islands are of tropical or temperate origins, where they were exposed to less stringent wind conditions. As wind likely represents a strong environmental filter for the successful establishment and further geographic spread of plants, they should have developed responses to resist and successfully colonize the Iles Kerguelen. We studied responses to wind of three herbaceous species that are invasive at Iles Kerguelen. We sampled plant individuals at different locations, under windy and sheltered conditions. Traits related to wind avoidance and tolerance and to resource acquisition were measured. We additionally assessed individual performance (biomass) to determine the consequences of trait variations. We focused on trait mean and variance, in particular, through the calculation of hypervolumes. This study emphasized that wind has important effects on plant economics spectrum, including traits involved in mechanical avoidance and light acquisition, with varying strategies, which seem to depend on the biological type of the species (grass versus non-grass). Wind generally reduces individual performance, and this negative effect is not direct but operates through the modification of plant trait values. Furthermore, analyses performed at the hypervolume scale indicate that not only functional trait mean but also its variability account for plant performance. The existence of contrasting growth strategies to cope with local environmental conditions suggests that invaders will be able to occupy different niches, which may ultimately impact local communities. Our results highlight the importance of considering multi-traits responses to meaningfully capture plant adjustments to stress. Â© 2021 Nordic Society Oikos. Published by John Wiley & Sons Ltd
Published: 2021

36. Parkinson’s disease with early motor complications: predicting EQ-5D- 3L utilities from PDQ-39 data in the EARLYSTIM trial

Author: W. M. Michael Schüpbach, Gillian Barnett, Isabelle Durand-Zaleski, Mehdi Zahra, Silke Walleser Autiero, Michal Górecki, Medtronic International Trading Sarl [Tolochenaz], Hôpital Hôtel-Dieu [Paris], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP), Service de santé publique [Mondor], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Hôpital Henri Mondor-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12), Health Technology Assessment Consulting [Kraków], Gillian Barnett and Associates [Dunfanaghy], Institut du Cerveau et de la Moëlle Epinière = Brain and Spine Institute (ICM), Institut National de la Santé et de la Recherche Médicale (INSERM)-CHU Pitié-Salpêtrière [AP-HP], Sorbonne Université (SU)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Service de neurologie 1 [CHU Pitié-Salpétrière], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-CHU Pitié-Salpêtrière [AP-HP], Sorbonne Université (SU)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU), Bern University Hospital [Berne] (Inselspital), Universität Bern [Bern], Centre d'investigation clinique Neurosciences [CHU Pitié Salpêtrière] (CIC Neurosciences), CHU Pitié-Salpêtrière [AP-HP], Sorbonne Université (SU)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP), Institut du Cerveau = Paris Brain Institute (ICM), Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Institut National de la Santé et de la Recherche Médicale (INSERM)-CHU Pitié-Salpêtrière [AP-HP], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU)-Sorbonne Université (SU)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Service de Neurologie [CHU Pitié-Salpêtrière], IFR70-CHU Pitié-Salpêtrière [AP-HP], Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU), Universität Bern [Bern] (UNIBE), Gestionnaire, Hal Sorbonne Université, Centre d'investigation clinique pluridisciplinaire [CHU Pitié Salpêtrière] (CIC-P 1421), and Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU)-Assistance publique - Hôpitaux de Paris (AP-HP) (AP-HP)-Sorbonne Université (SU)-Institut National de la Santé et de la Recherche Médicale (INSERM)-CHU Pitié-Salpêtrière [AP-HP]
Subjects: Male, Quality of life, medicine.medical_specialty, Parkinson's disease, Deep brain stimulation, medicine.medical_treatment, Cost-Benefit Analysis, lcsh:Computer applications to medicine. Medical informatics, 03 medical and health sciences, 0302 clinical medicine, Utility, EQ-5D, Surveys and Questionnaires, Post-hoc analysis, medicine, Humans, 030212 general & internal medicine, [SDV.NEU] Life Sciences [q-bio]/Neurons and Cognition [q-bio.NC], Multinomial logistic regression, [SDV.IB] Life Sciences [q-bio]/Bioengineering, business.industry, 030503 health policy & services, Research, Public Health, Environmental and Occupational Health, Parkinson Disease, General Medicine, Middle Aged, Physical Functional Performance, medicine.disease, [SDV.SPEE] Life Sciences [q-bio]/Santé publique et épidémiologie, Physical therapy, Parkinson’s disease, lcsh:R858-859.7, Female, [SDV.NEU]Life Sciences [q-bio]/Neurons and Cognition [q-bio.NC], [SDV.IB]Life Sciences [q-bio]/Bioengineering, [SDV.SPEE]Life Sciences [q-bio]/Santé publique et épidémiologie, Analysis of variance, Metric (unit), 0305 other medical science, business, Algorithms
Abstract: Background A utility value is a health-related quality of life metric (HRQoL) metric used in a cost-effectiveness analysis. While utilities as outcomes in the treatment of advanced Parkinson’s disease (PD) with deep brain stimulation (DBS) are available, they do not currently exist for PD with early motor complications. The objectives of this study were to predict utilities from observed disease-specific HRQoL data using two mapping algorithms, and investigate their performance in terms of longitudinal changes within and between treatment groups, and distribution by PD severity. Methods This is a post hoc analysis of data from the EARLYSTIM trial of DBS compared with best medical therapy (BMT) in PD patients with early motor complications We used two published algorithms comprising ordinal and multinomial regression models to map EQ-5D-3L utilities from observed PD-specific 39 item Questionnaire (PDQ-39) scores in EARLYSTIM. Utilities were calculated using the predicted functioning levels of EQ-5D-3L dimensions and the established EQ-5D-3L UK tariffs. Statistical analyses (analysis of variance, two-tailed Student’s t-test) were used to test the change from baseline within groups and difference in change from baseline between groups in utilities. Boxplots were developed to investigate the distribution of predicted utilities by PD severity, measured using the Hoehn and Yahr scale. Results The change from baseline in predicted mean utilities was statistically significant at all visits up to 24 months for the DBS group (p p = 0.04) for the BMT group with one algorithm. With both algorithms, the between-groups difference in change from baseline in predicted mean utilities favored DBS at all follow-up visits (p Conclusions Among PD patients with early motor complications, utilities predicted by both mapping algorithms using PDQ-39 data demonstrated a statistically and clinically meaningful improvement with DBS compared with BMT. It was not possible to conclude if one algorithm was more responsive than other. In the absence of utilities collected directly from patients, mapping is an acceptable option permitting economic evaluations to be undertaken.
Published: 2020

37. Stratigraphic architecture and depositional processes across lower Paleozoic siliciclastic shallow-marine platforms: insights from the Late Ordovician of the Anti-Atlas (Southern Morocco)

Author: Harlet, Déborah, Douillet, Guilhem, Ghienne, Jean Francois, Razin, Philippe, Dietrich, Pierre, Bouscary, Chloé, Schlunegger, Fritz, Institut für Geologie [Bern], Universität Bern [Bern], Ecole et Observatoire des Sciences de la Terre (EOST), Institut national des sciences de l'Univers (INSU - CNRS)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), ENSEGID, Géosciences Rennes (GR), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Rennes (OSUR)-Centre National de la Recherche Scientifique (CNRS), Institut des Dynamiques de la Surface Terrestre [Lausanne] (IDYST), Université de Lausanne (UNIL), Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Institut de physique du globe de Strasbourg (IPGS), Institut Polytechnique de Bordeaux (Bordeaux INP), Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Rennes (OSUR)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES), Dubigeon, Isabelle, Universität Bern [Bern] (UNIBE), Université de Rennes (UR)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Rennes (OSUR), Université de Rennes (UR)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Institut national des sciences de l'Univers (INSU - CNRS)-Université de Rennes 2 (UR2)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Centre National de la Recherche Scientifique (CNRS), and Université de Lausanne = University of Lausanne (UNIL)
Subjects: [SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/Stratigraphy, [SDU.STU.ST] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy, ComputingMilieux_MISCELLANEOUS
Abstract: International audience; During Cambrian-Ordovician times (542-444 Ma), the Anti-Atlas (Southern Morocco) was part of the Gondwana supercontinent and drifted from mid- to subpolar latitudes. The area was part of a shallow marine platform on the so-called northern passive margin of the continent. The stratigraphic succession records a long-term flooding of the platform from the Cambrian to the Silurian. Above Lower Cambrian fluvial to estuarine deposits, an essentially shallow-marine succession (from offshore shales to tidal sandstones) is punctuated by major flooding events in the Middle Cambrian, the lowermost Ordovician, the middle Ordovician and the lower Upper Ordovician. A superimposed eustatic sea-level drop due to the Late Ordovician glaciation marks the last transgressive-regressive cycle that includes the Ktaoua group (mid-Sandbian to Upper Katian) and the glaciation-related Second Bani Group (Hirnantian).In spite of well-known stratigraphy, details of the depositional processes, the overall geometry of the clinoforms (shelf vs. ramp) and resulting stacking patterns of the high-frequency units remain poorly understood in the platform domain. Here, we present a stratigraphic correlation made through a field-based logging of seven sections along a 50 km long, well-exposed cliff located in the Central Anti-Atlas. The Ktaoua to Second Bani groups, part of the Jbel Bani Mountain, are investigated between the villages of Tissint and Foum Zguid. The Ktaoua succession is dominated by high-order regressive parasequences grading from shales into fine to coarse-grained bioturbated sandstones, presenting paraconformable contacts. Incursions of sandstones showing hummocky-cross-stratifications (HCS) are common and considered to represent offshore-transition storm deposits. In the Second Bani Group, which includes glacially-related depositional facies (diamictites), fine to coarse-grained sandstones are dominant as well, though HCS are virtually absent. In the study area, the upper Second Bani Group forms an unconformable unit, severly truncating the Ktaoua succession and emphasizing a regressive sequence initiated within the Ktaoua deposition.These archives enable to constrain the basin geometry in the Upper Ordovician. Indeed, whereas offshore shales in the region of Zagora (Central Anti-Atlas) characterize the depocenter of the basin (eastward from the study area), the studied succession is surrounded by a belt of coarser-grained deposits to the north-east (Alnif, Eastern Anti-Atlas) and west (Tissint/Foum Zguid, Western Central Anti-Atlas). The stratigraphic correlation of the Ktaoua parasequences will be used to reconstruct the orientation, direction, and dip of platform clinoforms, which will allow to dissociate a scheme based on chronostratigraphic units from the usual lithostratigraphy. Besides, we aim to further characterize the geometry, shape, and stratigraphic position of HCS bodies in order to advance our understanding of the setting (e.g., paleobathymetry, position relative to regressive vs. transgressive trends) and hydrodynamic processes generating sandstones bodied with prevailing HCS beds.
Published: 2020

38. Future Missions related to the determination of the elemental and isotopic composition of Earth, Moon and the terrestrial planets

Author: Peter Wurz, Kristina G. Kislyakova, Iannis Dandouras, Michel Blanc, Eike W. Guenther, Yangting Lin, Helmut Lammer, Christian Mazelle, Shogo Tachibana, Manuel Scherf, Luca Fossati, Bernard Marty, Christophe Sotin, Laurenz Sproß, Sarah Rugheimer, M. Gerasimov, Masatoshi Yamauchi, Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Space Research Institute of Austrian Academy of Sciences (IWF), Austrian Academy of Sciences (OeAW), Space Research Institute of the Russian Academy of Sciences (IKI), Russian Academy of Sciences [Moscow] (RAS), Thüringer Landessternwarte Tautenburg (TLS), University of Vienna [Vienna], Chinese Academy of Sciences [Beijing] (CAS), Centre de Recherches Pétrographiques et Géochimiques (CRPG), Institut national des sciences de l'Univers (INSU - CNRS)-Université de Lorraine (UL)-Centre National de la Recherche Scientifique (CNRS), University of Oxford, Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Karl-Franzens-Universität Graz, Hokkaido University [Sapporo, Japan], Physikalisches Institut [Bern], Universität Bern [Bern] (UNIBE), Swedish Institute of Space Physics [Kiruna] (IRF), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), University of Oxford [Oxford], California Institute of Technology (CALTECH)-NASA, Karl-Franzens-Universität [Graz, Autriche], Universität Bern [Bern], Université de Lorraine (UL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), and University of Graz
Subjects: 010504 meteorology & atmospheric sciences, 530 Physics, [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], Planetary magnetospheres, 01 natural sciences, Space missions, Space exploration, Astrobiology, Planet, 0103 physical sciences, Terrestrial planets, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, Atmospheric escape, 520 Astronomy, Exoplanets, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy and Astrophysics, Mars Exploration Program, 620 Engineering, Exoplanet, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Planetary science, 13. Climate action, Space and Planetary Science, Physics::Space Physics, Environmental science, Terrestrial planet, Biosignatures, Astrophysics::Earth and Planetary Astrophysics, Planetary evolution, Exosphere, Planetary atmospheres
Abstract: In this chapter, we review the contribution of space missions to the determination of the elemental and isotopic composition of Earth, Moon and the terrestrial planets, with special emphasis on currently planned and future missions. We show how these missions are going to significantly contribute to, or sometimes revolutionise, our understanding of planetary evolution, from formation to the possible emergence of life. We start with the Earth, which is a unique habitable body with actual life, and that is strongly related to its atmosphere. The new wave of missions to the Moon is then reviewed, which are going to study its formation history, the structure and dynamics of its tenuous exosphere and the interaction of the Moon’s surface and exosphere with the different sources of plasma and radiation of its environment, including the solar wind and the escaping Earth’s upper atmosphere. Missions to study the noble gas atmospheres of the terrestrial planets, Venus and Mars, are then examined. These missions are expected to trace the evolutionary paths of these two noble gas atmospheres, with a special emphasis on understanding the effect of atmospheric escape on the fate of water. Future missions to these planets will be key to help us establishing a comparative view of the evolution of climates and habitability at Earth, Venus and Mars, one of the most important and challenging open questions of planetary science. Finally, as the detection and characterisation of exoplanets is currently revolutionising the scope of planetary science, we review the missions aiming to characterise the internal structure and the atmospheres of these exoplanets.
Published: 2020

39. Planetary system LHS 1140 revisited with ESPRESSO and TESS

Author: L. Acuña, Nathan Hara, Nuno C. Santos, David Barrado, João P. Faria, Emmanuel Marcq, Nicola Astudillo-Defru, Stéphane Udry, Xavier Bonfils, Francesco Pepe, Pedro Figueira, A. Leleu, Philippe Robutel, Alexandre C. M. Correia, Jorge Lillo-Box, S. G. Sousa, C. Lovis, Magali Deleuil, O. Mousis, Jose-Manuel Almenara, Centro de Astrobiologia [Madrid] (CAB), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC)-Instituto Nacional de Técnica Aeroespacial (INTA), European Southern Observatory [Santiago] (ESO), European Southern Observatory (ESO), Instituto de Astrofísica e Ciências do Espaço (IASTRO), Center for Space and Habitability (CSH), University of Bern, Space Research and Planetary Sciences [Bern) (WP), Physikalisches Institut [Bern], Universität Bern [Bern]-Universität Bern [Bern], National Centre of Competence in Research PlanetS (NCCR PlanetS), Universität Bern [Bern]-Universität Bern [Bern]-Swiss National Science Foundation (SNSF), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Departamento de Física e Astronomia [Porto] (DFA/FCUP), Faculdade de Ciências da Universidade do Porto (FCUP), Universidade do Porto-Universidade do Porto, Geneva Observatory, University of Geneva [Switzerland], Centro de Física da Universidade de Coimbra (CFisUC), Universidade de Coimbra [Coimbra], Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA), Departamento de Matemática y Fı́sica Aplicadas [Concepcion] (DMFA), Universidad Católica de la Santísima Concepción (UCSC), PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Spanish StateResearch Agency (AEI) Projects No.ESP2017-87676-C5-1-R and No. MDM-2017-0737 Unidad de Excelencia 'María de Maeztu' – Centro de Astrobiología(INTA-CSIC). This work was supported by FCT – Fundação para a Ciênciae a Tecnologia through national funds and by FEDER through COM-PETE2020 – Programa Operacional Competitividade e Internacionalizaçãoby these grants: UID/FIS/04434/2019, UIDB/04434/2020, UIDP/04434/2020, PTDC/FIS-AST/32113/2017 & POCI-01-0145-FEDER-032113, PTDC/FIS-AST/28953/2017 & POCI-01-0145-FEDER-028953. N.A.-D. acknowledges thesupport of FONDECYT project 3180063. X.B. and J.M.A. acknowledge fundingfrom the European Research Council under the ERC Grant Agreement n. 337591-ExTrA. A.C. acknowledges support by CFisUC projects (UIDB/04564/2020and UIDP/04564/2020), ENGAGE SKA (POCI-01-0145-FEDER-022217), andPHOBOS (POCI-01-0145-FEDER-029932), funded by COMPETE 2020 andFCT, Portugal. J.P.F. is supported in the form of a work contract funded bynational funds through FCT with reference DL57/2016/CP1364/CT0005, European Project: 337591,EC:FP7:ERC,ERC-2013-StG,EXTRA(2014), Instituto Nacional de Técnica Aeroespacial (INTA)-Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Universität Bern [Bern] (UNIBE)-Universität Bern [Bern] (UNIBE), Universität Bern [Bern] (UNIBE)-Universität Bern [Bern] (UNIBE)-Swiss National Science Foundation (SNSF), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Universidade do Porto = University of Porto-Universidade do Porto = University of Porto, Université de Genève = University of Geneva (UNIGE), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Faria, J. [0000-0002-6728-244X], Correia, A. C. M. [0000-0002-8946-8579], Leleu, A. [0000-0003-2051-7974], Lillo Box, J. [0000-0003-3742-1987], Santos, N. [0000-0003-4422-2919], Agencia Estatal de Investigación (AEI), FEDER through COMPETE2020 - Programa Operacional Competitividade e Internacionalizacao, Comisión Nacional de Investigación Científica y Tecnológica (CONICYT), European Research Council (ERC), ENGAGE SKA, PHOBOS, Portuguese Foundation for Science and Technology, Unidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737, Fundacao para a Ciencia e a Tecnologia (FCT), Fondo Nacional de Desarrollo Científico y Tecnológico (FONDECYT), and European Commission (EC)
Subjects: 010504 meteorology & atmospheric sciences, FOS: Physical sciences, Context (language use), Astrophysics, polarimetric [Techniques], 01 natural sciences, Photometry (optics), planets and satellites: terrestrial planets, Planet, 0103 physical sciences, techniques: radial velocities, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, Physics, Earth and Planetary Astrophysics (astro-ph.EP), [PHYS]Physics [physics], radial velocities [Techniques], planets and satellites: composition, Astronomy and Astrophysics, Planetary system, Orbital period, interiors [Planets and satellites], Exoplanet, planets and satellites: interiors, planets and satellites: individual: LHS1140, Radial velocity, techniques: polarimetric, 13. Climate action, Space and Planetary Science, terrestrial planets [Planets and satellites], composition [Planets and satellites], individual: LHS1140 [Planets and satellites], [SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA], [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Circumstellar habitable zone, Astrophysics - Earth and Planetary Astrophysics
Abstract: Context. LHS 1140 is an M dwarf known to host two transiting planets at orbital periods of 3.77 and 24.7 days. They were detected with HARPS and Spitzer. The external planet (LHS 1140 b) is a rocky super-Earth that is located in the middle of the habitable zone of this low-mass star. All these properties place this system at the forefront of the habitable exoplanet exploration, and it therefore constitutes a relevant case for further astrobiological studies, including atmospheric observations. Aims. We further characterize this system by improving the physical and orbital properties of the known planets, search for additional planetary-mass components in the system, and explore the possibility of co-orbitals. Methods. We collected 113 new high-precision radial velocity observations with ESPRESSO over a 1.5-yr time span with an average photon-noise precision of 1.07 m s-1. We performed an extensive analysis of the HARPS and ESPRESSO datasets and also analyzed them together with the new TESS photometry. We analyzed the Bayesian evidence of several models with different numbers of planets and orbital configurations. Results. We significantly improve our knowledge of the properties of the known planets LHS 1140 b (Pb ∼ 24.7 days) and LHS 1140 c (Pc ∼ 3.77 days). We determine new masses with a precision of 6% for LHS 1140 b (6.48 ± 0.46 Mpdbl) and 9% for LHS 1140 c (mc = 1.78 ± 0.17 Mpdbl). This reduces the uncertainties relative to previously published values by half. Although both planets have Earth-like bulk compositions, the internal structure analysis suggests that LHS 1140 b might be iron-enriched and LHS 1140 c might be a true Earth twin. In both cases, the water content is compatible to a maximum fraction of 10-12% in mass, which is equivalent to a deep ocean layer of 779 ± 650 km for the habitable-zone planet LHS 1140 b. Our results also provide evidence for a new planet candidate in the system (md = 4.8 ± 1.1Mpdbl) on a 78.9-day orbital period, which is detected through three independent methods. The analysis also allows us to discard other planets above 0.5 Mpdbl for periods shorter than 10 days and above 2 Mpdbl for periods up to one year. Finally, our co-orbital analysis discards co-orbital planets in the tadpole and horseshoe configurations of LHS 1140 b down to 1 Mpdbl with a 95% confidence level (twice better than with the previous HARPS dataset). Indications for a possible co-orbital signal in LHS 1140 c are detected in both radial velocity (alternatively explained by a high eccentricity) and photometric data (alternatively explained by systematics), however. Conclusions. The new precise measurements of the planet properties of the two transiting planets in LHS 1140 as well as the detection of the planet candidate LHS 1140 d make this system a key target for atmospheric studies of rocky worlds at different stellar irradiations., With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737)
Published: 2020

40. Change detection analyses using simulated and actual ExoMars TGO-CaSSIS images: A case study based on past and present Gasa Crater gully activity

Author: Alice Lucchetti, Frank P. Seelos, Manish R. Patel, Susan J. Conway, Nicolas Thomas, G. Munaretto, Maurizio Pajola, CaSSIS Team, Gabriele Cremonese, Vidhya Ganesh Rangarajan, Gordon R. Osinski, Livio L. Tornabene, Laboratoire de Planétologie et Géodynamique [UMR 6112] (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Space Research and Planetary Sciences [Bern) (WP), Physikalisches Institut [Bern], and Universität Bern [Bern]-Universität Bern [Bern]
Subjects: [SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology, Impact crater, biology, 13. Climate action, Cassis, [SDU.STU.GM]Sciences of the Universe [physics]/Earth Sciences/Geomorphology, biology.organism_classification, Geomorphology, ComputingMilieux_MISCELLANEOUS, Geology, Change detection
Abstract: Introduction: The Martian surface hosts a variety of active surface processes [1-3] whose regular monitoring is key to providing us insights into past and present-day surface, geologic and climatic conditions [4]. Most change detection studies on Mars utilize time-series image acquisitions from the Mars Reconnaissance Orbiter (MRO) High Resolution Imaging Science Experiment (HiRISE; 25-50 cm/px) [5] and the Context Camera (CTX; 5-6 m/px) [6]. However, the relatively narrow HiRISE colour swath (~20% of the image swath) results in a lower probability of observing surface changes with multiple wavelengths. The Colour and Stereo Surface Imaging System (CaSSIS) onboard the ExoMars Trace Gas Orbiter (TGO) [7] permits 4-band VNIR colour coverage at 4.6 m/px and an image swath >6 km. Furthermore, TGO/CaSSIS is able to observe Mars at multiple times of day, permitting detection/monitoring of diurnal processes. While TGO has only been in operation for a short period of time (MY34-35), the development of simulated CaSSIS images from MRO datasets [8] permits the monitoring of long-term surface changes with CaSSIS from as early as MY28 to present. This work assesses the change detection capabilities of CaSSIS by using a combination of simulated and actual CaSSIS images of one of the most active Martian gully sites to date – Gasa Crater [9-12] . Methods: We initially restricted the simulated CaSSIS images for this study to pre-2012 acquisitions, as our ability to fully photometrically correct CRISM targeted observations for along-track variations in emission/phase is confounded due to the loss of the full gimbal range of CRISM in late 2012 [8]. Three coordinated CRISM/CTX pairs were selected for production into simulated CaSSIS cubes based on a combination of favourable geometries, coverage, estimated atmospheric dust opacities and notable changes. Simulated CaSSIS images were generated using the procedures in [8] where spectrally and spatially resampled CaSSIS-compatible CRISM and CTX products are combined into a rigorous fully-simulated CaSSIS image using a Gram-Schmidt spectral pan-sharpening algorithm, which retains I/F information and minimises colour/spectral distortions [13]. To reduce atmospheric contributions, a dark-object-subtraction technique [14] was applied to both simulated and actual images. All images, including the first actual CaSSIS image acquired on Ls 350, MY34 were overlain and compared to one another to identify visible colour and/or morphologic changes. Notable changes were then compared with previously documented activity. Results and Discussion: We observe 28 possible changes between the simulated and actual CaSSIS image cubes spanning MY28 to MY34 (Fig. 1). Of these, 20 are previously undocumented changes, including 8 putative new changes and 12 fading flows (black-arrows in Fig. 1). All new/previously unrecognized changes are currently under active investigation with associated HiRISE coverage to verify if observed physical changes are not a manifestation of variable illumination conditions. Prominent changes previously observed between MY28 to 30 by [9,10] are all on the northern and north-eastern crater walls (red-arrows in Figs. 1a-c). While one prominent physical change (orange-arrow in Fig. 1c) was previously identified with a simulated CaSSIS image by [8], we note that 5 meter-scale physical changes noted by [9,10] are unresolved by CaSSIS products. Putative new colour changes are observed between MY29 and MY34 (Figs. 1, 2). Six of these were not readily visible with HiRISE due to lack of colour coverage. One prominent example includes a bright-bluish deposit in the eastern part of the crater (Figs. 1b-c). These deposits have an NIR-signature that suggests they are possible ferrous-bearing materials sourced from the gully alcoves [8,12,15]. The most-notable recent putative change based on our first CaSSIS acquisition of Gasa (Ls 350, MY34) shows a bright-bluish deposit on the eastern crater wall that spills partially onto the crater floor (Figs. 1d, 2). Although previous HiRISE acquisitions between MY31 and MY34 seem to show possible morphological changes, lack of HiRISE colour coverage over this deposit makes it difficult to verify the activity. A new optimally-positioned HiRISE acquisition later this year will enable us to verify this surface change (if it has not since faded). Conclusions: This study demonstrates how both simulated and actual CaSSIS cubes are useful for detecting both previously documented and potentially new gully activity at Gasa Crater. While CaSSIS may not capture all small meter-scale physical changes that HiRISE does, it allows for a much-improved colour-change capability over HiRISE. However, continuing to monitor with both instruments is pivotal, as CaSSIS detections of prominent colour changes can be used to reposition HiRISE to better target colour-coverage to validate and characterise meter-scale surface changes. Despite anticipated photometric complications that post-2012 CRISM targeted observations offer, future work will also include an assessment of simulated CaSSIS products generated with post-2012 CRISM and CTX coordinated data to assess identification of both new and previously documented HiRISE changes [16] after MY30. References: [1] McEwen et al. (2010), Icarus 205(1) [2] Bridges et al. (2013), Aeol. Res. 9 [3] Munaretto et al. (2020), PSS 187 [4] Greeley and Iversen (1985), Cambridge Univ. Press [5] McEwen et al. (2007), JGR 112 [6] Malin et al. (2007), JGR 112 [7] Thomas et al. (2017), SSR 212 [8] Tornabene et al. (2018), SSR 214(18) [9] Dundas et al. (2010), GRL 37 [10] Dundas et al. (2012), Icarus 220 [11] Dundas et al. (2015), Icarus 251 [12] Harrison et al. (2019), Geol. Soc. 467(1) [13] Laben et al. (2000), US Patent No: 6011875 [14] Chavez (1988), RSE 24(3) [15] Okubo et al. (2011), Icarus 211(1) [16] Dundas et al. (2019), Geol. Soc. 467(1). Acknowledgements: We thank the spacecraft and instrument engineering teams for the successful completion of the instrument. CaSSIS is a project of the University of Bern and funded through the Swiss Space Office via ESA's PRODEX programme. The instrument hardware development was also supported by the Italian Space Agency (ASI), INAF/Astronomical Observatory of Padova, and the Space Research Center (CBK) in Warsaw. Support from SGF (Budapest), the University of Arizona (Lunar and Planetary Lab.) and NASA are also gratefully acknowledged. The lead author acknowledges support from Tornabene’s funding from the CSA’s Planetary and Astronomy Missions Co-Investigator programme (19PACOI07) and the Canadian NSERC Discovery Grant programme (06418-2020 RGPIN).
Published: 2020

41. Detecting the elemental and molecular signatures of life: Laser-based mass spectrometry technologies ( A whitepaper written for the Planetary Science and Astrobiology Decadal Survey 2023–2032 of the National Academy of Sciences)

Author: Ligterink, Niels F.W., Riedo, Andreas, Tulej, Marek, Lukmanov, Rustam, Grimaudo, Valentine, De Koning, Coenraad, Wurz, Peter, Briois, Christelle, Carrasco, Nathalie, Jr., Ricardo Arevalo, Brinckerhoff, William B., Center for Space and Habitability (CSH), University of Bern, Space Research and Planetary Sciences [Bern) (WP), Physikalisches Institut [Bern], Universität Bern [Bern]-Universität Bern [Bern], Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National d’Études Spatiales [Paris] (CNES), Institut Universitaire de France (IUF), Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.), PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Department of Geology [College Park], University of Maryland [College Park], University of Maryland System-University of Maryland System, and NASA Goddard Space Flight Center (GSFC)
Subjects: [SDU]Sciences of the Universe [physics]
Abstract: The identification of extraterrestrial life is one the most exciting and challenging endeavors in space research. The existence of extinct or extant life can be inferred from biogenic elements, isotopes, and molecules, but accurate and sensitive instru- ments are needed to detect these species. In this whitepaper we show that Laser- based Mass Spectrometers are promising instrument for the in situ identification of atomic, isotopic, and molecular biosignatures. An overview of Laser abla- tion/Ionization Mass Spectrometry (LIMS) and Laser Desorption/Ionization Mass Spectrometry (LD-MS) instruments developed for space exploration is given. Their uses are discussed in the context of a Mars scenario and an Europa scenario. We show that Laser-based Mass Spectrometers are versatile and technologically ma- ture instruments with many beneficial characteristics for the detection of life. Fu- ture planetary lander and rover missions should be encouraged to make use of Laser-based Mass Spectrometry instruments in their scientific payload.
Published: 2020

42. AMBITION, the Comet Nucleus Cryogenic Sample Return mission for ESA Voyage 2050 program

Author: Filacchione, Gianrico, Bockelée-Morvan, Dominique, Altwegg, Kathrin, Bianchi, Eleonora, Bizzarro, Martin, Blum, Jürgen, Bonal, Lydie, Capaccioni, Fabrizio, Codella, Claudio, Choukroun, Mathieu, Cottin, Hervé, Davidsson, Björn, De Sanctis, Maria Cristina, Drozdovskaya, Maria, Engrand, Cécile, Galand, Marina, Güttler, Carsten, Henri, Pierre, Hérique, Alain, Ivanovski, Stavro L., Kokotanekova, Rosita, Levasseur-Regourd, Anny Chantal, Miller, Kelly E., Rotundi, Alessandra, Schönbächler, Maria, Snodgrass, Colin, Thomas, Nicolas, Tubiana, Cécilia, Ulamec, Stefan, Vincent, Jean-Baptiste, Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS), Istituto Nazionale di Astrofisica (INAF), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Physikalisches Institut [Bern], Universität Bern [Bern] (UNIBE), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France -Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France, Centre for Star and Planet Formation (STARPLAN), Globe Institute, Faculty of Health and Medical Sciences, University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH)-Faculty of Health and Medical Sciences, University of Copenhagen = Københavns Universitet (UCPH)-University of Copenhagen = Københavns Universitet (UCPH), Institut für Geophysik und Extraterrestrische Physik [Braunschweig] (IGEP), Technische Universität Braunschweig = Technical University of Braunschweig [Braunschweig], INAF - Osservatorio Astrofisico di Arcetri (OAA), Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Laboratoire Interuniversitaire des Systèmes Atmosphériques (LISA (UMR_7583)), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Center for Space and Habitability (CSH), University of Bern, Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Department of Physics [Imperial College London], Imperial College London, Max-Planck-Institut für Sonnensystemforschung (MPS), Max-Planck-Gesellschaft, Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), INAF - Osservatorio Astronomico di Trieste (OAT), European Southern Observatory [Garching], PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Southwest Research Institute [San Antonio] (SwRI), Department of Earth Sciences [Swiss Federal Institute of Technology - ETH Zürich] (D-ERDW), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Institute for Astronomy [Edinburgh] (IfA), University of Edinburgh, Deutsches Zentrum für Luft- und Raumfahrt [Köln] (DLR), DLR Institut für Planetenforschung, Deutsches Zentrum für Luft- und Raumfahrt [Berlin] (DLR), Cardon, Catherine, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Universität Bern [Bern], Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA), University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU)-Faculty of Health and Medical Sciences, University of Copenhagen = Københavns Universitet (KU)-University of Copenhagen = Københavns Universitet (KU), California Institute of Technology (CALTECH)-NASA, Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National d’Études Spatiales [Paris] (CNES), and Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)
Subjects: [SDU] Sciences of the Universe [physics], [SDU]Sciences of the Universe [physics], ComputingMilieux_MISCELLANEOUS
Abstract: International audience
Published: 2020

43. Characterizing brown dwarf companions with IRDIS long-slit spectroscopy: HD 1160 B and HD 19467 B

Author: Daniel Kitzmann, Valentina D'Orazi, Kevin Heng, Anne-Lise Maire, R. G. Gratton, Silvano Desidera, Mickael Bonnefoy, S. Peretti, Dino Mesa, Anthony Boccaletti, Baptiste Lavie, Arthur Vigan, Department of Biochemistry and Molecular Biology, Mayo Clinic, INAF - Osservatorio Astronomico di Padova (OAPD), Istituto Nazionale di Astrofisica (INAF), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Department of Geriatric Medicine, Centre Hospitalier Lyon Sud [CHU - HCL] (CHLS), Hospices Civils de Lyon (HCL)-Hospices Civils de Lyon (HCL), Physikalisches Institut [Bern], Universität Bern [Bern], Max-Planck-Institut für Astronomie (MPIA), Max-Planck-Gesellschaft, Observatoire Astronomique de l'Université de Genève (ObsGE), Université de Genève (UNIGE), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Universität Bern [Bern] (UNIBE), Université de Genève = University of Geneva (UNIGE), Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
Subjects: 010504 meteorology & atmospheric sciences, 530 Physics, Brown dwarf, FOS: Physical sciences, Astrophysics, 01 natural sciences, Spectral line, 0103 physical sciences, Angular resolution, Spectroscopy, infrared: planetary systems, 010303 astronomy & astrophysics, Solar and Stellar Astrophysics (astro-ph.SR), 0105 earth and related environmental sciences, Long-slit spectroscopy, instrumentation: spectrographs, Earth and Planetary Astrophysics (astro-ph.EP), Physics, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], 520 Astronomy, Astronomy and Astrophysics, Spectral bands, 500 Science, Surface gravity, methods: data analysis, Astrophysics - Solar and Stellar Astrophysics, Space and Planetary Science, techniques: imaging spectroscopy, Low Mass, Astrophysics - Earth and Planetary Astrophysics
Abstract: The determination of the fundamental properties (mass, separation, age, gravity and atmospheric properties) of brown dwarf companions allows us to infer crucial informations on their formation and evolution mechanisms. Spectroscopy of substellar companions is available to date only for a limited number of objects (and mostly at very low resolution, R, 14 pages, 14 Figures. Accepted for publication on MNRAS
Published: 2020

44. Zircon age of vaugnerite intrusives from the Central and Southern Vosges crystalline massif (E France): contribution to the geodynamics of the European Variscan belt

Author: Guillot, François, Averbuch, Olivier, Dubois, Michel, Durand, Cyril, Lanari, Pierre, Gauthier, Arnaud, Laboratoire d’Océanologie et de Géosciences (LOG) - UMR 8187 (LOG), Centre National de la Recherche Scientifique (CNRS)-Université du Littoral Côte d'Opale (ULCO)-Université de Lille-Institut national des sciences de l'Univers (INSU - CNRS), Laboratoire de Génie Civil et Géo-Environnement (LGCgE) - ULR 4515 (LGCgE), Université d'Artois (UA)-Université de Lille-Ecole nationale supérieure Mines-Télécom Lille Douai (IMT Lille Douai), Institut Mines-Télécom [Paris] (IMT)-Institut Mines-Télécom [Paris] (IMT)-JUNIA (JUNIA), Universität Bern [Bern], INSU-SYSTER program of the CNRS (DELAM project, PI O.A)., Institut national des sciences de l'Univers (INSU - CNRS)-Université du Littoral Côte d'Opale (ULCO)-Université de Lille-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD [France-Nord]), Université catholique de Lille (UCL)-Université catholique de Lille (UCL), and Universität Bern [Bern] (UNIBE)
Subjects: ultra-potassic magmatism, [SDU.STU.TE]Sciences of the Universe [physics]/Earth Sciences/Tectonics, [SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistry, syn-collisional lithospheric delamination, [SDU.STU.PE]Sciences of the Universe [physics]/Earth Sciences/Petrography, [SDU.STU]Sciences of the Universe [physics]/Earth Sciences, vaugnerites, Variscan orogeny, Vosges, Visean, [SDU.STU.MI]Sciences of the Universe [physics]/Earth Sciences/Mineralogy
Abstract: International audience; To provide a better picture of the active geodynamics along the Variscan suture zones during the late collisional stage (particularly regarding the evolution of the orogenic system towards HT conditions), we focused here on vaugnerites, which consist of mafic ultra-potassic magmatic rocks, intrusive into the granite-gneiss sequences of the Variscan Vosges crystalline massif. Those rocks, though subordinate in volume, are frequently associated with late-collisional granites. In the Central-Southern Vosges, they appear either as (1) pluton margin of the Southern Vosges Ballons granite complex or (2) composite dykes intrusive into migmatite and metamorphic sequences classically referred to as granite-gneiss unit (Central Vosges). Both types correspond to melanocratic rocks with prominent, Mg-rich, biotite and hornblende, two-feldspar and quartz. Those Vosges vaugnerites display geochemical signatures characteristic of ultra-potassic mafic to intermediate, metaluminous to slightly peraluminous rocks. Zircon U-Pb ages were obtained by Laser Ablation Inductively Coupled Plasma Mass Spectrometry. Zircon grains were extracted from a sillimanite-bearing gneiss from the granite-gneiss unit hosting the Central Vosges vaugnerites. They yielded an age at 451 ± 9 Ma, indicating a pre-Variscan Upper Ordovician protolith for the host sequence. Zircon from the four vaugnerite intrusives display U-Pb ages (± 2s) of 340 ± 2.5 Ma (Ballons), 340 ± 25 Ma, 340 ± 7 Ma and 336 ± 10 Ma (Central Vosges). Synchronous within uncertainty, vaugnerite age data suggest a relatively early emplacement during the Late Variscan collisional history (i.e. Middle Visean times). These results are in line with previously published ages from the Southern Vosges volcano-sedimentary sequences (Oderen-Markstein) and the nearby ultra-potassic granite complexes from the Central and Southern Vosges (Ballons, Crêtes) thereby arguing for a magmatic event of regional significance. Recent petrological studies on vaugnerites suggest that they derive from partial melting of a metasomatized mantle contaminated to some different degrees by elements of continental crust. We propose here that the major ultra-potassic magmatic pulse at 340-335 Ma is a consequence of a significant change into the dynamics of the Rhenohercynian subduction system below the Central-Southern Vosges. In the light of recent thermo-mechanical modelling experiments on mature continental collision, magmatism could result from a syn-collisional lithospheric delamination mechanism involving (1) first, continental subduction evolving towards (2) the underthrusting of the Avalonian continental margin lower crust and (3) the initiation of lithospheric delamination within the supra-subduction retro-wedge (Saxothuringian-Moldanubian continental block). This delamination would drive the emplacement of an asthenospheric upwelling, initially localized along the Variscan suture zones, and gradually propagating towards the southern front of the belt during the Late Carboniferous, as the delamination front migrated at the base of the crust.; Afin d’avancer dans la compréhension de la géodynamique des zones de suture varisque au stade tardif de la collision (en particulier au regard de l’évolution du système orogénique en contexte de HT), nous nous sommes intéressés à la mise en place des vaugnérites, roches basiques ultra-potassiques intrusives au sein des ensembles granito-gneissiques de la croûte varisque des Vosges. Ces roches, souvent associées aux ensembles granitiques tardi-collisionnels, sont de faible extension mais quasiment toujours présentes au sein de ces systèmes. Elles affleurent (1) dans les Vosges méridionales, en masses plutoniques marginales du Granite des Ballons et (2) dans les Vosges centrales (région de Plainfaing), en filons composites, intrusifs dans un complexe de migmatites et de roches métamorphiques appelées granite-gneiss. Les vaugnérites sont des roches mélanocrates à biotite et hornblende magnésiennes, présentant des signatures géochimiques caractéristiques de roches ultra-potassiques mafiques à intermédiaires, métalumineuses à légèrement peralumineuses. L’âge U-Pb obtenu par ablation laser ICP-MS du zircon d’un gneiss à sillimanite du granite-gneiss encaissant des vaugnérites est de 451 ± 9 Ma, révélant un bâti pré-varisque à protolithe ordovicien supérieur. Les grains de zircon extraits de quatre vaugnérites donnent des âges U-Pb (± 2sigma) de 340 ± 2,5 Ma (Ballons), 340 ± 25 Ma, 340 ± 7Ma et 336 ± 10Ma (Vosges centrales). Les données de datation des vaugnérites, identiques aux incertitudes de mesure près, apparaissent donc cohérentes et révèlent un âge assez précoce dans l’histoire tardi-collisionnelle de la chaîne. Ces données, en accord avec les âges publiés préalablement sur ce secteur, montrent que les vaugnérites se mettent en place au Viséen moyen, au cours d’un événement magmatique majeur, exprimé tant dans les séries volcano-sédimentaires (Séries Oderen- Markstein) que dans les granitoïdes ultra-potassiques des Vosges méridionales (Ballons) et centrales (Crêtes). Les études pétrologiques récentes sur les vaugnérites suggèrent qu’elles dérivent de la fusion partielle d’un manteau métasomatisé et contaminé à différents degrés par des éléments de croûte continentale fondue. Nous proposons ici que ce « pulse » magmatique ultra-potassique d’ampleur à 340– 335 Ma soit le signe une évolution majeure dans la dynamique de la subduction de la lithosphère rhénohercynienne sous les Vosges centrales et méridionales. Sur le modèle d’expériences thermomécaniques récentes simulant le déroulement d’une collision continentale mature, il pourrait traduire les premiers effets d’un phénomène de délamination lithosphérique syn-collisionelle impliquant (1) une subduction continentale relayée (2) par le sous-charriage d’une lame de croûte inférieure de la marge continentale avalonienne et (3) l’initiation de la délamination lithosphérique au sein du prisme orogénique supra-subduction qu’était le bloc continental saxothüringien-moldanubien. Ce processus conduirait à la mise en place d’un « upwelling » asthénosphérique, initialement localisé aux zones de suture varisque et se propageant au cours de la fin du Carbonifère vers le front sud de la chaîne à mesure de la propagation du front de délamination à la base de la croûte.
Published: 2020

45. A Diiron Hydrogenase Mimic Featuring a 1,2,3-Triazolylidene

Author: Martin Albrecht, Philippe Schollhammer, Catherine Elleouet, Simone Bertini, François Y. Pétillon, Andrea Mele, Chimie, Electrochimie Moléculaires et Chimie Analytique (CEMCA), Institut Brestois Santé Agro Matière (IBSAM), Université de Brest (UBO)-Université de Brest (UBO)-Centre National de la Recherche Scientifique (CNRS)-Institut de Chimie du CNRS (INC), Universität Bern [Bern], CNRS (Centre National de la Recherche Scientifique), the Université de Bretagne Occidentale, are also acknowl-edged for financial support., European Project: 675020,H2020,H2020-MSCA-ITN-2015,NoNoMeCat(2016), Université de Brest (UBO)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Institut Brestois Santé Agro Matière (IBSAM), Université de Brest (UBO), and Universität Bern [Bern] (UNIBE)
Subjects: Proton, 010405 organic chemistry, Mesoionic carbene, Mesoionic, proton reductions, General Medicine, General Chemistry, Hydrogenase mimic, [CHIM.INOR]Chemical Sciences/Inorganic chemistry, 010402 general chemistry, 01 natural sciences, Combinatorial chemistry, Bioinspired model, 3. Good health, 0104 chemical sciences, lcsh:Chemistry, chemistry.chemical_compound, Proton reduction, chemistry, lcsh:QD1-999, Hydrogenase, [CHIM]Chemical Sciences, Cyclic voltammetry, Diiron complex, Carbene
Abstract: A novel complex featuring a mesoionic carbene [Fe2(CO)5(trz)(?-pdt)] (1) (trz = 1-phenyl-l,3-methyl,4-butyl-1,2,3-triazol-5-ylidene), was synthesized and spectroscopically and structurally characterized. The reductive behaviour of this compound in the presence and in the absence of acid (CH3CO2H) was examined by cyclic voltammetry (CV) that revealed the lack of efficient activity towards proton reduction.
Published: 2020

46. How to implement a fair and progressive carbon price to fight climate change?

Author: Boroumand, Raphaël-Homayoun, Goutte, Stéphane, Porcher, Thomas, Stocker, Thomas, City University London, Centre d'études sur la mondialisation, les conflits, les territoires et les vulnérabilités (Cemotev), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ), Paris School of Business (PSB), National Centre of Competence in Research PlanetS (NCCR PlanetS), Swiss National Science Foundation (SNSF)-Physikalisches Institut [Bern], and Universität Bern [Bern]-Universität Bern [Bern]
Subjects: [SHS.STAT]Humanities and Social Sciences/Methods and statistics, carbon, [SHS.ENVIR]Humanities and Social Sciences/Environmental studies, market, tax, [SHS.ECO]Humanities and Social Sciences/Economics and Finance, climate, price
Abstract: The principle of "common but differentiated responsibility", a key concept of the United Nations Framework Convention on Climate Change (UNFCCC), acknowledges the conditions for a generally acceptable and differentiated pricing mechanism on carbon emissions. With reference to this principle, carbon price determination has become one of the necessary instruments to limit global warming to a maximum of 2 °C. In this article, we propose the allocation of a carbon price per country based on the Human Development Index (HDI) and 0 2 emissions per capita. We demonstrate that under a multilateral framework, the price of carbon would be fixed according to a reference price depending on the HDI and 0 2 emissions. For example, if a country emits more than the amount allocated to its HDI level, it will have to pay a higher price than the established reference price, and vice versa. Reference prices as functions of HDIs and emissions will be estimated based on a trajectory to reach the target goal of reducing carbon dioxide emissions. A key element of our proposed scheme is that it generates national revenue allowing high-emitting countries a rapid decarbonization and developing countries (with generally lower emissions) accelerated development and early implementation of green infrastructures. Our research goal is related to documenting the benefits of a differentiated and progressive carbon pricing mechanism to ease intergovernmental cooperation.
Published: 2020

47. The Deep Composition of Uranus and Neptune from In Situ Exploration and Thermochemical Modeling

Author: Peter Wurz, Michel Dobrijevic, Roda Bounaceur, Jérémy Leconte, Thibault Cavalié, Yamila Miguel, Olivia Venot, Olivier Mousis, Leigh N. Fletcher, Vincent Hue, Laboratoire d'Astrophysique de Bordeaux [Pessac] (LAB), Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), ASP 2020, Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Bordeaux (UB)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics (LESIA), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire Interuniversitaire des Systèmes Atmosphériques (LISA (UMR_7583)), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut Pierre-Simon-Laplace (IPSL (FR_636)), École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-Centre National d'Études Spatiales [Toulouse] (CNES)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Leiden Observatory [Leiden], Universiteit Leiden, School of Physics and Astronomy [Leicester], University of Leicester, Physikalisches Institut [Bern], Universität Bern [Bern] (UNIBE), Univers, Transport, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) (UTINAM), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC), Laboratoire Réactions et Génie des Procédés (LRGP), Université de Lorraine (UL)-Centre National de la Recherche Scientifique (CNRS), Southwest Research Institute [San Antonio] (SwRI), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Est Créteil Val-de-Marne - Paris 12 (UPEC UP12)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Universiteit Leiden [Leiden], Universität Bern [Bern], Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), and Centre National de la Recherche Scientifique (CNRS)-Université de Lorraine (UL)
Subjects: Solar System, 010504 meteorology & atmospheric sciences, Gas giant, [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], FOS: Physical sciences, 01 natural sciences, law.invention, Astrobiology, Orbiter, [CHIM.GENI]Chemical Sciences/Chemical engineering, law, Neptune, 0103 physical sciences, 14. Life underwater, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, ComputingMilieux_MISCELLANEOUS, 0105 earth and related environmental sciences, [INFO.INFO-SC]Computer Science [cs]/Symbolic Computation [cs.SC], Earth and Planetary Astrophysics (astro-ph.EP), [INFO.INFO-PL]Computer Science [cs]/Programming Languages [cs.PL], Uranus, Astronomy and Astrophysics, [INFO.INFO-MO]Computer Science [cs]/Modeling and Simulation, Planetary science, 13. Climate action, Space and Planetary Science, Great conjunction, Astrophysics - Instrumentation and Methods for Astrophysics, Ice giant, Geology, Astrophysics - Earth and Planetary Astrophysics
Abstract: The distant ice giants of the Solar System, Uranus and Neptune, have only been visited by one space mission, Voyager 2. The current knowledge on their composition remains very limited despite some recent advances. A better characterization of their composition is however essential to constrain their formation and evolution, as a significant fraction of their mass is made of heavy elements, contrary to the gas giants Jupiter and Saturn. An in situ probe like Galileo would provide us with invaluable direct ground-truth composition measurements. However, some of the condensibles will remain out of the grasp of a shallow probe. While additional constraints could be obtained from a complementary orbiter, thermochemistry and diffusion modeling can further help us to increase the science return of an in situ probe., Comment: Accepted for publication in Space Science Reviews
Published: 2020

48. Impact of Morphology on Charge Carrier Transport and Thermoelectric Properties of N‐Type FBDOPV‐Based Polymers

Author: Alexandre Carella, Renaud Demadrille, Tamara Nunes Domschke, Wojciech Pisula, Serge Gambarelli, Martina Sandroni, Paweł Kubik, Benjamin Grévin, Pawel Veyre, Stéphanie Pouget, Tomasz Marszalek, Asma Aicha Medjahed, Olivier Bardagot, Universität Bern [Bern], Łódź University of Technology, Synthèse, Structure et Propriétés de Matériaux Fonctionnels (STEP ), SYstèmes Moléculaires et nanoMatériaux pour l’Energie et la Santé (SYMMES), Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes (UGA)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes (UGA), Département Interfaces pour l'énergie, la Santé et l'Environnement (DIESE), Institut Laue-Langevin (ILL), ILL, Service Général des Rayons X (SGX ), Modélisation et Exploration des Matériaux (MEM), Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes (UGA)-Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Laboratoire d'Innovation pour les Technologies des Energies Nouvelles et les nanomatériaux (LITEN), Institut National de L'Energie Solaire (INES), Centre National de la Recherche Scientifique (CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Centre National de la Recherche Scientifique (CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Département des Technologies des NanoMatériaux (DTNM), Centre National de la Recherche Scientifique (CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Centre National de la Recherche Scientifique (CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de L'Energie Solaire (INES), Conception d’Architectures Moléculaires et Processus Electroniques (CAMPE ), ANR-16-CE05-0029,Harvesters,Récuperer l'energie thermique de l'environnement à l'aide d'un générateur thermoélectrique polymère pour alimenter un capteur autonome(2016), Universität Bern [Bern] (UNIBE), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de L'Energie Solaire (INES)
Subjects: chemistry.chemical_classification, Morphology (linguistics), Materials science, [CHIM.ORGA]Chemical Sciences/Organic chemistry, [SPI.NRJ]Engineering Sciences [physics]/Electric power, 02 engineering and technology, Polymer, 010402 general chemistry, 021001 nanoscience & nanotechnology, Condensed Matter Physics, 01 natural sciences, 0104 chemical sciences, Electronic, Optical and Magnetic Materials, Biomaterials, Organic semiconductor, [CHIM.POLY]Chemical Sciences/Polymers, chemistry, Chemical engineering, Thermoelectric effect, Electrochemistry, [SPI.MECA.THER]Engineering Sciences [physics]/Mechanics [physics.med-ph]/Thermics [physics.class-ph], [CHIM]Chemical Sciences, Charge carrier, 0210 nano-technology
Abstract: International audience; The impact of the chemical structure and molecular order on the charge transport properties of two donor–acceptor copolymers in their neutral anddoped states is investigated. Both polymers comprise 3,7-bis((E)-7-fluoro-1-(2-octyl-dodecyl)-2-oxoindolin-3-ylidene)-3,7-dihydrobenzo[1,2-b:4,5-b′]difuran-2,6-dione (FBDOPV) as electron-accepting unit, copolymerized with 9,9-dioctyl-fluorene (P(FBDOPV-F)) or with 3-dodecyl-2,2′-bithiophene(P(FBDOPV-2T-C12)). These copolymers possess an amorphous and semicrystalline nature, respectively, and exhibit remarkable electron mobilities of 0.065 and 0.25 cm2 V–1 s–1 in field effect transistors. However, after chemical n-doping with 4-(1,3-dimethyl-2,3-dihydro-1H-benzoimidazol-2-yl)phenyl) dimethylamine (N-DMBI), electrical conductivities four orders of magnitude higher can be achieved for P(FBDOPV-2T-C12) (σ = 0.042 S cm−1). More charge-transfer complexes are formed between P(FBDOPV-F) and N-DMBI, but the highly localized polaronic states poorly contribute to the charge transport. Doped P(FBDOPV-2T-C12) exhibits a negative Seebeck coefficient of –265 μV K−1 and a thermoelectric power factor (PF) of 0.30 μW m−1 K−2 at 303 K which increases to 0.72 μW m−1 K−2 at 388 K. The in-plane thermal conductivity (κ|| = 0.53 W m−1 K−1) on the same micrometer-thick solution-processed film is measured, resulting in a figure of merit (ZT) of 5.0 × 10−4 at 388 K. The results provide important design guidelines to improve the doping efficiency and thermoelectric properties of n-type organic semiconductors.
Published: 2020

49. CINeMA: An approach for assessing confidence in the results of a network meta-analysis

Author: Matthias Egger, Theodoros Papakonstantinou, Adriani Nikolakopoulou, Cinzia Del Giovane, Julian P T Higgins, Anna Chaimani, Georgia Salanti, Institute of Social and Preventive Medicine [Bern] (ISPM), Universität Bern [Bern] (UNIBE), University of Bristol [Bristol], Centre de Recherche Épidémiologie et Statistique Sorbonne Paris Cité (CRESS (U1153 / UMR_A_1125 / UMR_S_1153)), Conservatoire National des Arts et Métiers [CNAM] (CNAM), HESAM Université - Communauté d'universités et d'établissements Hautes écoles Sorbonne Arts et métiers université (HESAM)-HESAM Université - Communauté d'universités et d'établissements Hautes écoles Sorbonne Arts et métiers université (HESAM)-Université Sorbonne Paris Cité (USPC)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université Paris Cité (UPCité)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), Cochrane France [Paris], University of Bern, Institute of Primary Health Care, The development of the software and part of the presented work was supported by the Cochrane Collaboration and the Campbell Collaboration. GS, AN, TP were supported by project funding (Grant No. 179158) from the Swiss National Science Foundation. ME was supported by special project funding (Grant No. 174281) from the Swiss National Science Foundation., Bodescot, Myriam, Universität Bern [Bern], and Conservatoire National des Arts et Métiers [CNAM] (CNAM)-Université Sorbonne Paris Cité (USPC)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université de Paris (UP)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)
Subjects: Computer science, Network Meta-Analysis, Coronary Artery Disease, 030204 cardiovascular system & hematology, computer.software_genre, Vascular Medicine, Diagnostic Radiology, Guidelines and Guidance, Electrocardiography, Mathematical and Statistical Techniques, 0302 clinical medicine, Credibility, Medicine and Health Sciences, Coronary Heart Disease, 030212 general & internal medicine, 610 Medicine & health, Randomized Controlled Trials as Topic, Radiology and Imaging, Statistics, Drugs, General Medicine, Transparency (human–computer interaction), Metaanalysis, Magnetic Resonance Imaging, Bioassays and Physiological Analysis, Reporting bias, Research Design, Meta-analysis, Physical Sciences, Medicine, Network Analysis, 360 Social problems & social services, Computer and Information Sciences, Imaging Techniques, Clinical Research Design, Process (engineering), Cardiology, Magnetic Resonance Imaging, Cine, Research and Analysis Methods, Machine learning, 03 medical and health sciences, Diagnostic Medicine, Confidence Intervals, Humans, Web application, Statistical Methods, Pharmacology, business.industry, Electrophysiological Techniques, Statins, Confidence interval, [SDV.SPEE] Life Sciences [q-bio]/Santé publique et épidémiologie, Exercise Test, Key (cryptography), [SDV.SPEE]Life Sciences [q-bio]/Santé publique et épidémiologie, Cardiac Electrophysiology, Adverse Events, Artificial intelligence, business, computer, Mathematics
Abstract: Background The evaluation of the credibility of results from a meta-analysis has become an important part of the evidence synthesis process. We present a methodological framework to evaluate confidence in the results from network meta-analyses, Confidence in Network Meta-Analysis (CINeMA), when multiple interventions are compared. Methodology CINeMA considers 6 domains: (i) within-study bias, (ii) reporting bias, (iii) indirectness, (iv) imprecision, (v) heterogeneity, and (vi) incoherence. Key to judgments about within-study bias and indirectness is the percentage contribution matrix, which shows how much information each study contributes to the results from network meta-analysis. The contribution matrix can easily be computed using a freely available web application. In evaluating imprecision, heterogeneity, and incoherence, we consider the impact of these components of variability in forming clinical decisions. Conclusions Via 3 examples, we show that CINeMA improves transparency and avoids the selective use of evidence when forming judgments, thus limiting subjectivity in the process. CINeMA is easy to apply even in large and complicated networks., Adriani Nikolakopoulou and co-authors discuss CINeMA, an approach for evaluating the findings of network meta-analyses.
Published: 2020

50. Dysfunction of homeostatic control of dopamine by astrocytes in the developing prefrontal cortex leads to cognitive impairments

Author: Corrado Calì, Tamara Zehnder, Graham Knott, Sébastien Sultan, Luca Pucci, Cedric S. Asensio, Robert H. Edwards, Paola Bezzi, Nicole Déglon, Francesco Petrelli, Andrei Ivanov, Glenn Dallérac, Vidar Gundersen, Andrea Chicca, Jürg Gertsch, Nicolas Toni, Jean-Pierre Mothet, Salvatore Lecca, Frank Kirchhoff, Bruno Giros, Fulvio Magara, Department of Fundamental Neurosciences, [University of Lausanne], Université de Lausanne (UNIL), Centre de recherche en neurobiologie - neurophysiologie de Marseille (CRN2M), Aix Marseille Université (AMU)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Lumière, Matière et Interfaces (LuMIn), CentraleSupélec-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Ecole Normale Supérieure Paris-Saclay (ENS Paris Saclay), Université de Lausanne = University of Lausanne (UNIL), Institut des Neurosciences Paris-Saclay (NeuroPSI), Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), University of Naples Federico II = Università degli studi di Napoli Federico II, Centre de recherche en neurosciences de Lyon - Lyon Neuroscience Research Center (CRNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Université Jean Monnet - Saint-Étienne (UJM)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS), Institut du Fer à Moulin, Institut National de la Santé et de la Recherche Médicale (INSERM)-Sorbonne Université (SU), Universität Bern [Bern] (UNIBE), Laboratoire de Photonique Quantique et Moléculaire (LPQM), École normale supérieure - Cachan (ENS Cachan)-CentraleSupélec-Centre National de la Recherche Scientifique (CNRS), University of California [San Francisco] (UC San Francisco), University of California (UC), Division of Anatomy [Oslo], Department of Molecular Medicine [Oslo], Institute of Basic Medical Sciences [Oslo], Faculty of Medicine [Oslo], University of Oslo (UiO)-University of Oslo (UiO)-Faculty of Medicine [Oslo], University of Oslo (UiO)-University of Oslo (UiO)-Institute of Basic Medical Sciences [Oslo], University of Oslo (UiO)-University of Oslo (UiO), Ecole Polytechnique Fédérale de Lausanne (EPFL), Saarland University [Saarbrücken], Centre Hospitalier Universitaire Vaudois [Lausanne] (CHUV), Neuroscience Paris Seine (NPS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut de Biologie Paris Seine (IBPS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS), éTICC, Laboratoire Aimé Cotton (LAC), École normale supérieure - Cachan (ENS Cachan)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Cachan (ENS Cachan)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Università degli studi di Napoli Federico II, Centre de recherche en neurosciences de Lyon (CRNL), Université de Lyon-Université de Lyon-Université Jean Monnet [Saint-Étienne] (UJM)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS), Universität Bern [Bern], Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-École normale supérieure - Cachan (ENS Cachan)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-École normale supérieure - Cachan (ENS Cachan)-Laboratoire de Photonique Quantique et Moléculaire (LPQM), École normale supérieure - Cachan (ENS Cachan)-CentraleSupélec-Centre National de la Recherche Scientifique (CNRS)-CentraleSupélec-Centre National de la Recherche Scientifique (CNRS), University of California [San Francisco] (UCSF), University of California, Neurosciences Paris Seine (NPS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Institut de Biologie Paris Seine (IBPS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-École normale supérieure - Cachan (ENS Cachan)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-École normale supérieure - Cachan (ENS Cachan), Centre interdisciplinaire de recherche en biologie (CIRB), Collège de France (CdF)-Institut National de la Santé et de la Recherche Médicale (INSERM)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Institut des Neurosciences de Paris-Saclay (Neuro-PSI), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Mathematics and Computing in Automatic Control and Optimization for the User (MIAOU), Inria Sophia Antipolis - Méditerranée (CRISAM), Institut National de Recherche en Informatique et en Automatique (Inria)-Institut National de Recherche en Informatique et en Automatique (Inria), Institut National de la Santé et de la Recherche Médicale (INSERM)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de neurobiologie cellulaire et moléculaire (NBCM), and Centre National de la Recherche Scientifique (CNRS)
Subjects: Male, 0301 basic medicine, Physiology, [SDV.NEU.NB]Life Sciences [q-bio]/Neurons and Cognition [q-bio.NC]/Neurobiology, [SDV]Life Sciences [q-bio], astrocytes, dopamine, VMAT2, neurons, monoamine transporter, Vesicular monoamine transporter 2, Synaptic Transmission, Rats, Sprague-Dawley, Mice, 0302 clinical medicine, synaptic-transmission, Homeostasis, 610 Medicine & health, Prefrontal cortex, Mice, Knockout, biology, Executive functions, Psychiatry and Mental health, Excitatory postsynaptic potential, [SDV.NEU]Life Sciences [q-bio]/Neurons and Cognition [q-bio.NC], Neural development, medicine.drug, MESH: Neuroscience, brain, Prefrontal Cortex, clearance, Neurotransmission, Article, 03 medical and health sciences, Cellular and Molecular Neuroscience, Dopamine, expression, medicine, Animals, Cognitive Dysfunction, gene, Molecular Biology, MESH: Physiology, organic cation transporter-3, proteins, Rats, 030104 developmental biology, biology.protein, 570 Life sciences, central-nervous-system, Neuroscience, 030217 neurology & neurosurgery
Abstract: International audience; Astrocytes orchestrate neural development by powerfully coordinating synapse formation and function and, as such, may be critically involved in the pathogenesis of neurodevelopmental abnormalities and cognitive deficits commonly observed in psychiatric disorders. Here, we report the identification of a subset of cortical astrocytes that are competent for regulating dopamine (DA) homeostasis during postnatal development of the prefrontal cortex (PFC), allowing for optimal DA-mediated maturation of excitatory circuits. Such control of DA homeostasis occurs through the coordinated activity of astroglial vesicular monoamine transporter 2 (VMAT2) together with organic cation transporter 3 and monoamine oxidase type B, two key proteins for DA uptake and metabolism. Conditional deletion of VMAT2 in astrocytes postnatally produces loss of PFC DA homeostasis, leading to defective synaptic transmission and plasticity as well as impaired executive functions. Our findings show a novel role for PFC astrocytes in the DA modulation of cognitive performances with relevance to psychiatric disorders.
Published: 2020

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