1,463 results on '"Galeazzi, M."'
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2. The scar: the wind in the perfect storm—insights into the mysterious living tissue originating ventricular arrhythmias
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Pandozi, C., Mariani, Marco Valerio, Chimenti, C., Maestrini, V., Filomena, D., Magnocavallo, M., Straito, M., Piro, A., Russo, M., Galeazzi, M., Ficili, S., Colivicchi, F., Severino, P., Mancone, M., Fedele, F., and Lavalle, C.
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- 2023
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3. Ultra-high density mapping for the evaluation of the antral scar extension after ablation with a radiofrequency balloon catheter in atrial fibrillation patients
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Poggi, S, primary, Almorad, A, additional, Pandozzi, C, additional, Torri, F, additional, Strisciuglio, T, additional, Iuliano, A, additional, Russo, M, additional, Manfrin, M, additional, Galeazzi, M, additional, Bertagnolli, L, additional, Spiniello, G, additional, Stabile, G, additional, and Chierchia, G B, additional
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- 2024
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4. The Structure of the Local Hot Bubble
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Liu, W., Chiao, M., Collier, M. R., Cravens, T., Galeazzi, M., Koutroumpa, D., Kuntz, K. D., Lallement, R., Lepri, S. T., McCammon, D., Morgan, K., Porter, F. S., Snowden, S. L., Thomas, N. E., Uprety, Y., Ursino, E., and Walsh, B. M.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
DXL (Diffuse X-rays from the Local Galaxy) is a sounding rocket mission designed to quantify and characterize the contribution of Solar Wind Charge eXchange (SWCX) to the Diffuse X-ray Background and study the properties of the Local Hot Bubble (LHB). Based on the results from the DXL mission, we quantified and removed the contribution of SWCX to the diffuse X-ray background measured by the ROSAT All Sky Survey (RASS). The "cleaned" maps were used to investigate the physical properties of the LHB. Assuming thermal ionization equilibrium, we measured a highly uniform temperature distributed around kT=0.097 keV+/-0.013 keV (FWHM)+/-0.006 keV (systematic). We also generated a thermal emission measure map and used it to characterize the three-dimensional (3D) structure of the LHB which we found to be in good agreement with the structure of the local cavity measured from dust and gas., Comment: 8 pages, 10 figures, Accepted for publication on ApJ
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- 2016
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5. Solar Wind Charge Exchange contribution to the ROSAT All Sky Survey Maps
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Uprety, Y., Chiao, M., Collier, M. R., Cravens, T., Galeazzi, M., Koutroumpa, D., Kuntz, K. D., Lallement, R., Lepri, S. T., Liu, W., McCammon, D., Morgan, K., Porter, F. S., Prasai, K., Snowden, S. L., Thomas, N. E., Ursino, E., and Walsh, B. M.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Solar and Stellar Astrophysics - Abstract
DXL (Diffuse X-ray emission from the Local Galaxy) is a sounding rocket mission designed to estimate the contribution of Solar Wind Charge eXchange (SWCX) to the Diffuse X-ray Background (DXB) and to help determine the properties of the Local Hot Bubble (LHB). The detectors are large-area thin-window proportional counters with a spectral response similar to that of the PSPC used in the ROSAT All Sky Survey (RASS). A direct comparison of DXL and RASS data for the same part of the sky viewed from quite different vantage points in the Solar system and the assumption of approximate isotropy for the Solar wind allowed us to quantify the SWCX contribution to all 6 RASS bands (R1-R7, excepting R3). We find that the SWCX contribution at l=140 deg, b=0 deg, where the DXL path crosses the Galactic plane is 33%+-6% (statistical)+-12%(systematic) for R1, 44%+-\%+-5% for R2, 18%+-12%+-11% for R4, 14%+-11%+-9% for R5, and negligible for R6 and R7 bands. Reliable models for the distribution of neutral H and He in the Solar system permit estimation of the contribution of interplanetary SWCX emission over the the whole sky and correction of the RASS maps. We find that the average SWCX contribution in the whole sky is 26%+-6%+-13% for R1, 30%+-4%+-4% for R2, 8%+-5%+-5% for R4, 6%+-4%+-4% for R5, and negligible for R6 and R7., Comment: 9 pages, 13 figures, accepted for publication on ApJ
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- 2016
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6. Studying the Interstellar Medium and the inner region of NPS/Loop 1 with shadow observations toward MBM36
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Ursino, E., Galeazzi, M., and Liu, W.
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Astrophysics - Astrophysics of Galaxies ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
We analyzed data from a shadow observation of the high density molecular cloud MBM36 (l~4{\deg}, b~35{\deg}) with Suzaku. MBM36 is located in a region that emits relatively weakly in the 3/4~keV band, compared to the surrounding NPS/Loop 1 structure and the Galactic Bulge. The contrast between a high and low density targets in the MBM36 area allows one to separate the local and distant contributors to the Soft Diffuse X-ray Background, providing a much better characterization of the individual components compared to single pointing observations. We identify two non-local thermal components, one at kT~0.12 keV and one at kT~0.29keV. The colder component matches well with models of emission from the higher latitude region of the Galactic Bulge. The emission of the warmer component is in agreement with models predicting that the NPS is due to a hypershell from the center of the Milky Way. Geometrical and pressure calculations rule out a nearby bubble as responsible for the emission associate with the NPS. Any Galactic Halo/CircumGalactic Halo emission, if present, is outshined by the other components. We also report an excess emission around 0.9~keV, likely due to an overabundance of NeIX., Comment: 8 pages, 3 figures, approved for publication on ApJ
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- 2015
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7. Exploring the bridge between A3556 and A3558 in the Shapley Supercluster
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Ursino, E., Galeazzi, M., Gupta, A., Kelley, R., Mitsuishi, I., Ohashi, T., and Sato, K.
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Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Astrophysics of Galaxies - Abstract
Looking at the region connecting two clusters is a promising way to identify and study the Warm-Hot Intergalactic Medium. Observations show that the spectrum of the bridge between A3556 and A3558 has a stronger soft X-ray emission than the nearby region. Suzaku observations could not discriminate the origin of the extra emission. In this work we analyze a dedicated Chandra observation of the same target to identify point sources and characterize the background emission in the bridge. We find that the count number of the point sources is much higher than average field population (using CDFS~4~Ms as a reference). Moreover, the shape of the cumulative distribution resembles that of galaxy distribution suggesting that the point sources are galaxies in a filament. The Suzaku extra emission is well explained by the high abundance of point sources identified by Chandra. Furthermore, we used optical/IR observations of point sources in the same field to estimate the density of the putative filament as rho~150 rho_b$, below Suzaku sensitivity., Comment: 6 pages, 4 figures, accepted for publication on ApJ
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- 2015
8. The Intermediate Neutrino Program
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Adams, C., Alonso, J. R., Ankowski, A. M., Asaadi, J. A., Ashenfelter, J., Axani, S. N., Babu, K., Backhouse, C., Band, H. R., Barbeau, P. S., Barros, N., Bernstein, A., Betancourt, M., Bishai, M., Blucher, E., Bouffard, J., Bowden, N., Brice, S., Bryan, C., Camilleri, L., Cao, J., Carlson, J., Carr, R. E., Chatterjee, A., Chen, M., Chen, S., Chiu, M., Church, E. D., Collar, J. I., Collin, G., Conrad, J. M., Convery, M. R., Cooper, R. L., Cowen, D., Davoudiasl, H., De Gouvea, A., Dean, D. J., Deichert, G., Descamps, F., DeYoung, T., Diwan, M. V., Djurcic, Z., Dolinski, M. J., Dolph, J., Donnelly, B., Dwyer, D. A., Dytman, S., Efremenko, Y., Everett, L. L., Fava, A., Figueroa-Feliciano, E., Fleming, B., Friedland, A., Fujikawa, B. K., Gaisser, T. K., Galeazzi, M., Galehouse, D. C., Galindo-Uribarri, A., Garvey, G. T., Gautam, S., Gilje, K. E., Gonzalez-Garcia, M., Goodman, M. C., Gordon, H., Gramellini, E., Green, M. P., Guglielmi, A., Hackenburg, R. W., Hackenburg, A., Halzen, F., Han, K., Hans, S., Harris, D., Heeger, K. M., Herman, M., Hill, R., Holin, A., Huber, P., Jaffe, D. E., Johnson, R. A., Joshi, J., Karagiorgi, G., Kaufman, L. J., Kayser, B., Kettell, S. H., Kirby, B. J., Klein, J. R., Kolomensky, Yu. G., Kriske, R. M., Lane, C. E., Langford, T. J., Lankford, A., Lau, K., Learned, J. G., Ling, J., Link, J. M., Lissauer, D., Littenberg, L., Littlejohn, B. R., Lockwitz, S., Lokajicek, M., Louis, W. C., Luk, K., Lykken, J., Marciano, W. J., Maricic, J., Markoff, D. M., Caicedo, D. A. Martinez, Mauger, C., Mavrokoridis, K., McCluskey, E., McKeen, D., McKeown, R., Mills, G., Mocioiu, I., Monreal, B., Mooney, M. R., Morfin, J. G., Mumm, P., Napolitano, J., Neilson, R., Nelson, J. K., Nessi, M., Norcini, D., Nova, F., Nygren, D. R., Gann, G. D. Orebi, Palamara, O., Parsa, Z., Patterson, R., Paul, P., Pocar, A., Qian, X., Raaf, J. L., Rameika, R., Ranucci, G., Ray, H., Reyna, D., Rich, G. C., Rodrigues, P., Romero, E. Romero, Rosero, R., Rountree, S. D., Rybolt, B., Sanchez, M. C., Santucci, G., Schmitz, D., Scholberg, K., Seckel, D., Shaevitz, M., Shrock, R., Smy, M. B., Soderberg, M., Sonzogni, A., Sousa, A. B., Spitz, J., John, J. M. St., Stewart, J., Strait, J. B., Sullivan, G., Svoboda, R., Szelc, A. M., Tayloe, R., Thomson, M. A., Toups, M., Vacheret, A., Vagins, M., Van de Water, R. G., Vogelaar, R. B., Weber, M., Weng, W., Wetstein, M., White, C., White, B. R., Whitehead, L., Whittington, D. W., Wilking, M. J., Wilson, R. J., Wilson, P., Winklehner, D., Winn, D. R., Worcester, E., Yang, L., Yeh, M., Yokley, Z. W., Yoo, J., Yu, B., Yu, J., and Zhang, C.
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High Energy Physics - Experiment ,Nuclear Experiment ,Physics - Instrumentation and Detectors - Abstract
The US neutrino community gathered at the Workshop on the Intermediate Neutrino Program (WINP) at Brookhaven National Laboratory February 4-6, 2015 to explore opportunities in neutrino physics over the next five to ten years. Scientists from particle, astroparticle and nuclear physics participated in the workshop. The workshop examined promising opportunities for neutrino physics in the intermediate term, including possible new small to mid-scale experiments, US contributions to large experiments, upgrades to existing experiments, R&D plans and theory. The workshop was organized into two sets of parallel working group sessions, divided by physics topics and technology. Physics working groups covered topics on Sterile Neutrinos, Neutrino Mixing, Neutrino Interactions, Neutrino Properties and Astrophysical Neutrinos. Technology sessions were organized into Theory, Short-Baseline Accelerator Neutrinos, Reactor Neutrinos, Detector R&D and Source, Cyclotron and Meson Decay at Rest sessions.This report summarizes discussion and conclusions from the workshop., Comment: pdfLaTeX, 31 pages, 1 figure, minor modification to 0nuBB discussion
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- 2015
9. ASTRO-H White Paper - Clusters of Galaxies and Related Science
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Kitayama, T., Bautz, M., Markevitch, M., Matsushita, K., Allen, S., Kawaharada, M., McNamara, B., Ota, N., Akamatsu, H., de Plaa, J., Galeazzi, M., Madejski, G., Main, R., Miller, E., Nakazawa, K., Russell, H., Sato, K., Sekiya, N., Simionescu, A., Tamura, T., Uchida, Y., Ursino, E., Werner, N., Zhuravleva, I., and ZuHone, J.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
The next generation X-ray observatory ASTRO-H will open up a new dimension in the study of galaxy clusters by achieving for the first time the spectral resolution required to measure velocities of the intracluster plasma, and extending at the same time the spectral coverage to energies well beyond 10 keV. This white paper provides an overview of the capabilities of ASTRO-H for exploring gas motions in galaxy clusters including their cosmological implications, the physics of AGN feedback, dynamics of cluster mergers as well as associated high-energy processes, chemical enrichment of the intracluster medium, and the nature of missing baryons and unidentified dark matter., Comment: 92 pages, 52 figures, ASTRO-H White Paper
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- 2014
10. ASTRO-H White Paper - New Spectral Features
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Smith, R. K., Odaka, H., Audard, M., Brown, G. V., Eckart, M. E., Ezoe, Y., Foster, A., Galeazzi, M., Hamaguchi, K., Ishibashi, K., Ishikawa, K., Kaastra, J., Katsuda, S., Leutenegger, M., Miller, E., Mitsuishi, I., Nakajima, H., Ogawa, T., Paerels, F., Porter, F. S., Sakai, K., Sawada, M., Takei, Y., Tanaka, Y., Tsuboi, Y., Uchida, H., Ursino, E., Watanabe, S., Yamaguchi, H., and Yamasaki, N.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
This white paper addresses selected new (to X-ray astronomy) physics and data analysis issues that will impact ASTRO-H SWG observations as a result of its high-spectral-resolution X-ray microcalorimeter, the focussing hard X-ray optics and corresponding detectors, and the low background soft gamma-ray detector. We concentrate on issues of atomic and nuclear physics, including basic bound-bound and bound-free transitions as well as scattering and radiative transfer. The major topic categories include the physics of charge exchange, solar system X-ray sources, advanced spectral model, radiative transfer, and hard X-ray emission lines and sources., Comment: 37 pages, 19 figures, ASTRO-H White Paper
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- 2014
11. The origin of the 'local' 1/4 keV X-ray flux in both charge exchange and a hot bubble
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Galeazzi, M., Chiao, M., Collier, M. R., Cravens, T., Koutroumpa, D., Kuntz, K. D., Lallement, R., Lepri, S. T., McCammon, D., Morgan, K., Porter, F. S., Robertson, I. P., Snowden, S. L., Thomas, N. E., Uprety, Y., Ursino, E., and Walsh, B. M.
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Astrophysics - Solar and Stellar Astrophysics - Abstract
The Solar neighborhood is the closest and most easily studied sample of the Galactic interstellar medium, an understanding of which is essential for models of star formation and galaxy evolution. Observations of an unexpectedly intense diffuse flux of easily-absorbed 1/4 keV X rays, coupled with the discovery that interstellar space within ~100 pc of the Sun is almost completely devoid of cool absorbing gas led to a picture of a "local cavity" filled with X-ray emitting hot gas dubbed the local hot bubble. This model was recently upset by suggestions that the emission could instead be produced readily within the solar system by heavy solar wind ions charge exchanging with neutral H and He in interplanetary space, potentially removing the major piece of evidence for the existence of million-degree gas within the Galactic disk. Here we report results showing that the total solar wind charge exchange contribution is 40% +/- 5% (stat) +/- 5% (sys) of the 1/4 keV flux in the Galactic plane. The fact that the measured flux is not dominated by charge exchange supports the notion of a million-degree hot bubble of order 100 pc extent surrounding the Sun., Comment: 9 pages, 6 figures, 1 table. The final version of the paper is available on Nature
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- 2014
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12. The Intermediate Neutrino Program
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Adams, C, Alonso, JR, Ankowski, AM, Asaadi, JA, Ashenfelter, J, Axani, SN, Babu, K, Backhouse, C, Band, HR, Barbeau, PS, Barros, N, Bernstein, A, Betancourt, M, Bishai, M, Blucher, E, Bouffard, J, Bowden, N, Brice, S, Bryan, C, Camilleri, L, Cao, J, Carlson, J, Carr, RE, Chatterjee, A, Chen, M, Chen, S, Chiu, M, Church, ED, Collar, JI, Collin, G, Conrad, JM, Convery, MR, Cooper, RL, Cowen, D, Davoudiasl, H, Gouvea, A De, Dean, DJ, Deichert, G, Descamps, F, DeYoung, T, Diwan, MV, Djurcic, Z, Dolinski, MJ, Dolph, J, Donnelly, B, Dwyer, DA, Dytman, S, Efremenko, Y, Everett, LL, Fava, A, Figueroa-Feliciano, E, Fleming, B, Friedland, A, Fujikawa, BK, Gaisser, TK, Galeazzi, M, Galehouse, DC, Galindo-Uribarri, A, Garvey, GT, Gautam, S, Gilje, KE, Gonzalez-Garcia, M, Goodman, MC, Gordon, H, Gramellini, E, Green, MP, Guglielmi, A, Hackenburg, RW, Hackenburg, A, Halzen, F, Han, K, Hans, S, Harris, D, Heeger, KM, Herman, M, Hill, R, Holin, A, Huber, P, Jaffe, DE, Johnson, RA, Joshi, J, Karagiorgi, G, Kaufman, LJ, Kayser, B, Kettell, SH, Kirby, BJ, Klein, JR, Kolomensky, Yu G, Kriske, RM, Lane, CE, Langford, TJ, Lankford, A, Lau, K, Learned, JG, Ling, J, Link, JM, Lissauer, D, Littenberg, L, Littlejohn, BR, and Lockwitz, S
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hep-ex ,nucl-ex ,physics.ins-det - Abstract
The US neutrino community gathered at the Workshop on the IntermediateNeutrino Program (WINP) at Brookhaven National Laboratory February 4-6, 2015 toexplore opportunities in neutrino physics over the next five to ten years.Scientists from particle, astroparticle and nuclear physics participated in theworkshop. The workshop examined promising opportunities for neutrino physics inthe intermediate term, including possible new small to mid-scale experiments,US contributions to large experiments, upgrades to existing experiments, R&Dplans and theory. The workshop was organized into two sets of parallel workinggroup sessions, divided by physics topics and technology. Physics workinggroups covered topics on Sterile Neutrinos, Neutrino Mixing, NeutrinoInteractions, Neutrino Properties and Astrophysical Neutrinos. Technologysessions were organized into Theory, Short-Baseline Accelerator Neutrinos,Reactor Neutrinos, Detector R&D and Source, Cyclotron and Meson Decay at Restsessions.This report summarizes discussion and conclusions from the workshop.
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- 2015
13. Probing the anisotropy of the Milky Way gaseous halo: Sight-lines toward Mrk 421 and PKS2155-304
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Gupta, A., Mathur, S., Galeazzi, M., and Krongold, Y.
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Astrophysics - Astrophysics of Galaxies - Abstract
(Abridged) We recently found that the halo of the Milky Way contains a large reservoir of warm-hot gas that contains a large fraction of the missing baryons from the Galaxy. The average physical properties of this circumgalactic medium (CGM) are determined by combining average absorption and emission measurements along several extragalactic sightlines. However, there is a wide distribution of both, the halo emission measure and the \ovii column density, suggesting that the Galactic warm-hot gaseous halo is anisotropic. We present {\it Suzaku} observations of fields close to two sightlines along which we have precise \ovii absorption measurements with \chandran. The column densities along these two sightlines are similar within errors, but we find that the emission measures are different. Therefore the densities and pathlengths in the two directions must be different, providing a suggestive evidence that the warm-hot gas in the CGM of the Milky Way is not distributed uniformly. However, the formal errors on derived parameters are too large to make such a claim. The average density and pathlength of the two sightlines are similar to the global averages, so the halo mass is still huge, over 10 billion solar masses. With more such studies, we will be able to better characterize the CGM anisotropy and measure its mass more accurately. We also show that the Galactic disk makes insignificant contribution to the observed \ovii absorption; a similar conclusion was also reached independently about the emission measure. We further argue that any density inhomogeneity in the warm-hot gas, be it from clumping, from the disk, or from a non-constant density gradient, would strengthen our result in that the Galactic halo path-length and the mass would become larger than what we estimate here. As such, our results are conservative and robust., Comment: 27 pages, 5 figures, submitted to ApJ
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- 2013
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14. Observed Limits on Charge Exchange Contributions to the Diffuse X-ray Background
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Crowder, S. G., Barger, K. A., Brandl, D. E., Eckart, M. E., Galeazzi, M., Kelley, R. L., Kilbourne, C. A., McCammon, D., Pfendner, C. G., Porter, F. S., Rocks, L., Szymkowiak, A. E., and Teplin, I. M.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Galaxy Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics ,Physics - Space Physics - Abstract
We present a high resolution spectrum of the diffuse X-ray background from 0.1 to 1 keV for a ~1 region of the sky centered at l=90, b=+60 using a 36-pixel array of microcalorimeters flown on a sounding rocket. With an energy resolution of 11 eV FWHM below 1 keV, the spectrum's observed line ratios help separate charge exchange contributions originating within the heliosphere from thermal emission of hot gas in the interstellar medium. The X-ray sensitivity below 1 keV was reduced by about a factor of four from contamination that occurred early in the flight, limiting the significance of the results. The observed centroid of helium-like O VII is 568+2-3 eV at 90% confidence. Since the centroid expected for thermal emission is 568.4 eV while for charge exchange is 564.2 eV, thermal emission appears to dominate for this line complex, consistent with much of the high-latitude O VII emission originating in 2-3 x 10^6 K gas in the Galactic halo. On the other hand, the observed ratio of C VI Ly gamma to Ly alpha is 0.3+-0.2. The expected ratios are 0.04 for thermal emission and 0.24 for charge exchange, indicating that charge exchange must contribute strongly to this line and therefore potentially to the rest of the ROSAT R12 band usually associated with 10^6 K emission from the Local Hot Bubble. The limited statistics of this experiment and systematic uncertainties due to the contamination require only >32% thermal emission for O VII and >20% from charge exchange for C VI at the 90% confidence level. An experimental gold coating on the silicon substrate of the array greatly reduced extraneous signals induced on nearby pixels from cosmic rays passing through the substrate, reducing the triggered event rate by a factor of 15 from a previous flight of the instrument., Comment: 14 pages, 7 figures, to be published in ApJ
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- 2012
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15. Reconstructing the shape of the correlation function
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Huffenberger, K. M., Galeazzi, M., and Ursino, E.
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Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
We develop an estimator for the correlation function which, in the ensemble average, returns the shape of the correlation function, even for signals that have significant correlations on the scale of the survey region. Our estimator is general and works in any number of dimensions. We develop versions of the estimator for both diffuse and discrete signals. As an application, we examine Monte Carlo simulations of X-ray background measurements. These include a realistic, spatially-inhomogeneous population of spurious detector events. We discuss applying the estimator to the averaging of correlation functions evaluated on several small fields, and to other cosmological applications., Comment: 10 pages, 5 figures, submitted to ApJS. Methods and results unchanged but text is expanded and significantly reordered in response to referee
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- 2012
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16. A huge reservoir of ionized gas around the Milky Way: Accounting for the Missing Mass?
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Gupta, A., Mathur, S., Krongold, Y., Nicastro, F., and Galeazzi, M.
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Most of the baryons from galaxies have been "missing" and several studies have attempted to map the circumgalactic medium (CGM) of galaxies in their quest. Recent studies with the Hubble Space Telescope have shown that many galaxies contain a large reservoir of ionized gas with temperatures of about 10^5 K. Here we report on X-ray observations made with the Chandra X-ray Observatory probing an even hotter phase of the CGM of our Milky Way at about 10^6 K. We show that this phase of the CGM is massive, extending over a large region around the Milky Way, with a radius of over 100 kpc. The mass content of this phase is over ten billion solar masses, many times more than that in cooler gas phases and comparable to the total baryonic mass in the disk of the Galaxy. The missing mass of the Galaxy appears to be in this warm-hot gas phase., Comment: 15 pages, 3 figures; http://stacks.iop.org/2041-8205/756/L8
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- 2012
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17. DXL: a sounding rocket mission for the study of solar wind charge exchange and local hot bubble X-ray emission
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Galeazzi, M., Chiao, M., Collier, M. R., Cravens, T., Koutroumpa, D., Kuntz, K. D., Lepri, S., McCammon, D., Porter, F. S., Prasai, K., Robertson, I., Snowden, S., and Uprety, Y.
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Astrophysics - Solar and Stellar Astrophysics - Abstract
The Diffuse X-rays from the Local galaxy (DXL) mission is an approved sounding rocket project with a first launch scheduled around December 2012. Its goal is to identify and separate the X-ray emission generated by solar wind charge exchange from that of the local hot bubble to improve our understanding of both. With 1,000 cm2 proportional counters and grasp of about 10 cm2 sr both in the 1/4 and 3/4 keV bands, DXL will achieve in a 5-minute flight what cannot be achieved by current and future X-ray satellites., Comment: 15 Pages, 5 figures. Accepted for publication on Experimental Astronomy
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- 2011
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18. ORIGIN: Metal Creation and Evolution from the Cosmic Dawn
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Herder, J. W. den, Piro, L., Ohashi, T., Kouveliotou, C., Hartmann, D. H., Kaastra, J. S., Amati, L., Andersen, M. I., Arnaud, M., Attéia, J-L., Bandler, S., Barbera, M., Barcons, X., Barthelmy, S., Basa, S., Basso, S., Boer, M., Branchini, E., Branduardi-Raymont, G., Borgani, S., Boyarsky, A., Brunetti, G., Budtz-Jorgensen, C., Burrows, D., Butler, N., Campana, S., Caroli, E., Ceballos, M., Christensen, F., Churazov, E., Comastri, A., Colasanti, L., Cole, R., Content, R., Corsi, A., Costantini, E., Conconi, P., Cusumano, G., de Plaa, J., De Rosa, A., Del Santo, M., Di Cosimo, S., De Pasquale, M., Doriese, R., Ettori, S., Evans, P., Ezoe, Y., Ferrari, L., Finger, H., Figueroa-Feliciano, T., Friedrich, P., Fujimoto, R., Furuzawa, A., Fynbo, J., Gatti, F., Galeazzi, M., Gehrels, N., Gendre, B., Ghirlanda, G., Ghisellini, G., Gilfanov, M., Giommi, P., Girardi, M., Grindlay, J., Cocchi, M., Godet, O., Guedel, M., Haardt, F., Hartog, R. den, Hepburn, I., Hermsen, W., Hjorth, J., Hoekstra, H., Holland, A., Hornstrup, A., van der Horst, A., Hoshino, A., Zand, J. in 't, Irwin, K., Ishisaki, Y., Jonker, P., Kitayama, T., Kawahara, H., Kawai, N., Kelley, R., Kilbourne, C., de Korte, P., Kusenko, A., Kuvvetli, I., Labanti, M., Macculi, C., Maiolino, R., Hesse, M. Mas, Matsushita, K., Mazzotta, P., McCammon, D., Méndez, M., Mignani, R., Mineo, T., Mitsuda, K., Mushotzky, R., Molendi, S., Moscardini, L., Natalucci, L., Nicastro, F., O'Brien, P., Osborne, J., Paerels, F., Page, M., Paltani, S., Pedersen, K., Perinati, E., Ponman, T., Pointecouteau, E., Predehl, P., Porter, S., Rasmussen, A., Rauw, G., Röttgering, H., Roncarelli, M., Rosati, P., Quadrini, E., Ruchayskiy, O., Salvaterra, R., Sasaki, S., Sato, K., Savaglio, S., Schaye, J., Sciortino, S., Shaposhnikov, M., Sharples, R., Shinozaki, K., Spiga, D., Sunyaev, R., Suto, Y., Takei, Y., Tanvir, N., Tashiro, M., Tamura, T., Tawara, Y., Troja, E., Tsujimoto, M., Tsuru, T., Ubertini, P., Ullom, J., Ursino, E., Verbunt, F., van de Voort, F., Viel, M., Wachter, S., Watson, D., Weisskopf, M., Werner, N., White, N., Willingale, R., Wijers, R., Yamasaki, N., Yoshikawa, K., and Zane, S.
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Astrophysics - Instrumentation and Methods for Astrophysics ,Astrophysics - Cosmology and Extragalactic Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
ORIGIN is a proposal for the M3 mission call of ESA aimed at the study of metal creation from the epoch of cosmic dawn. Using high-spectral resolution in the soft X-ray band, ORIGIN will be able to identify the physical conditions of all abundant elements between C and Ni to red-shifts of z=10, and beyond. The mission will answer questions such as: When were the first metals created? How does the cosmic metal content evolve? Where do most of the metals reside in the Universe? What is the role of metals in structure formation and evolution? To reach out to the early Universe ORIGIN will use Gamma-Ray Bursts (GRBs) to study their local environments in their host galaxies. This requires the capability to slew the satellite in less than a minute to the GRB location. By studying the chemical composition and properties of clusters of galaxies we can extend the range of exploration to lower redshifts (z ~ 0.2). For this task we need a high-resolution spectral imaging instrument with a large field of view. Using the same instrument, we can also study the so far only partially detected baryons in the Warm-Hot Intergalactic Medium (WHIM). The less dense part of the WHIM will be studied using absorption lines at low redshift in the spectra for GRBs., Comment: 34 pages, 13 figures. ESA Cosmic Vision medium-class mission (M3) proposal. Accepted for publication in Experimental Astronomy. Including minor corrections in the author list
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- 2011
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19. Properties of the Diffuse X-ray Background toward MBM20 with Suzaku
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Gupta, A., Galeazzi, M., Koutroumpa, D., Smith, R., and Lallement, R.
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Astrophysics - Galaxy Astrophysics ,Astrophysics - Solar and Stellar Astrophysics - Abstract
We used Suzaku observations of the molecular cloud MBM20 and a low neutral hydrogen column density region nearby to separate and characterize the foreground and background diffuse X-ray emission. A comparison with a previous observation of the same regions with XMM-Newton indicates a significant change in the foreground flux which is attributed to Solar Wind Charge eXchange (SWCX). The data have also been compared with previous results from similar "shadow" experiments and with a SWCX model to characterize its O VII and O VIII emission., Comment: Accepted for publication in ApJ; 29 pages, 7 figures
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- 2009
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20. Studying the WHIM with Gamma Ray Bursts
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Branchini, E., Ursino, E., Corsi, A., Martizzi, D., Amati, L., Herder, J. W. den, Galeazzi, M., Gendre, B., Kaastra, J., Moscardini, L., Nicastro, F., Ohashi, T., Paerels, F., Piro, L., Roncarelli, M., Takei, Y., and Viel, M.
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Astrophysics - Cosmology and Extragalactic Astrophysics - Abstract
We assess the possibility to detect and characterize the physical state of the missing baryons at low redshift by analyzing the X-ray absorption spectra of the Gamma Ray Burst [GRB] afterglows, measured by a micro calorimeters-based detector with 3 eV resolution and 1000 cm2 effective area and capable of fast re-pointing, similar to that on board of the recently proposed X-ray satellites EDGE and XENIA. For this purpose we have analyzed mock absorption spectra extracted from different hydrodynamical simulations used to model the properties of the Warm Hot Intergalactic Medium [WHIM]. These models predict the correct abundance of OVI absorption lines observed in UV and satisfy current X-ray constraints. According to these models space missions like EDGE and XENIA should be able to detect about 60 WHIM absorbers per year through the OVII line. About 45 % of these have at least two more detectable lines in addition to OVII that can be used to determine the density and the temperature of the gas. Systematic errors in the estimates of the gas density and temperature can be corrected for in a robust, largely model-independent fashion. The analysis of the GRB absorption spectra collected in three years would also allow to measure the cosmic mass density of the WHIM with about 15 % accuracy, although this estimate depends on the WHIM model. Our results suggest that GRBs represent a valid, if not preferable, alternative to Active Galactic Nuclei to study the WHIM in absorption. The analysis of the absorption spectra nicely complements the study of the WHIM in emission that the spectrometer proposed for EDGE and XENIA would be able to carry out thanks to its high sensitivity and large field of view., Comment: 16 pages, 16 figures, accepted for publication by ApJ
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- 2009
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21. Evidence for the Missing Baryons in the Angular Correlation of the Diffuse X-ray Background
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Galeazzi, M., Gupta, A., and Ursino, E.
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Astrophysics - Abstract
The amount of detected baryons in the local Universe is at least a factor of two smaller than measured at high redshift. It is believed that a significant fraction of the baryons in the current Universe is "hiding" in a hot filamentary structure filling the intergalactic space, the Warm-Hot Intergalactic Medium ($WHIM$). We found evidence of the missing baryons in the $WHIM$ by detecting their signature on the angular correlation of diffuse X-ray emission with the XMM-Newton satellite. Our result indicates that $(12\pm 5)$% of the total diffuse X-ray emission in the energy range 0.4-0.6 keV is due to intergalactic filaments. The statistical significance of our detection is several sigmas ($\chi ^2>136$ N=19). The error bar in the X-ray flux is dominated, instead, by cosmic variation and model uncertainties., Comment: 15 pages, 3 figures, Accepted for publication on ApJ
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- 2008
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22. Xmm-Newton Observations of the Diffuse X-ray Background
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Galeazzi, M., Gupta, A., Covey, K., and Ursino, E.
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Astrophysics - Abstract
We analyzed two XMM-Newton observations in the direction of the high density, high latitude, neutral hydrogen cloud MBM20 and of a nearby low density region that we called the Eridanus hole. The cloud MBM20 is at a distance evaluated between 100 and 200 pc from the Sun and its density is sufficiently high to shield about 75% of the foreground emission in the 3/4 keV energy band.The combination of the two observations makes possible an evaluation of the OVII and OVIII emission both for the foreground component due to the Local Bubble,and the background one, due primary to the galactic halo.The two observations are in good agreement with each other and with ROSAT observations of the same part of the sky and the OVII and OVIII fluxes are OVII=3.89+/-0.56 photons cm^-2 s^-1 sr^-1, OVIII=0.68+/-0.24 photons cm^-2 s^-1 sr^-1 for MBM20 and OVII=7.26+/-0.34 photons cm^-2 s^-1 sr^-1,OVIII=1.63+/-0.17 photons cm^-2 s^-1 sr^-1 for the Eridanus hole. The spectra are in agreement with a simple three component model, one unabsorbed and one absorbed plasma component, and a power law, without evidence for any strong contamination from ion exchange in the solar system. Assuming that the two plasma components are in thermal equilibrium we obtain a temperature of 0.096 keV for the foreground component and 0.197 keV for the background one. Assuming the foreground component is due solely to Local Bubble emission we obtain a lower and upper limit for the plasma density of 0.0079 cm^-3 and 0.0095 cm^-3 and limits of 16,200 cm^-3 K and 19,500 cm^-3 K for the plasma pressure, in good agreement with theoretical predictions. Similarly, assuming that the absorbed plasma component is due to Galactic halo emission, we obtain a plasma density ranging from 0.0009 cm^-3 to 0.0016 cm^-3, and a pressure ranging from 3.0*10^3 to 6.7*10^3 cm^-3 K., Comment: 31 pages, 5 figures, Accepted for publication in ApJ
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- 2006
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23. X-Ray Emission from the Warm Hot Intergalactic Medium
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Ursino, E. and Galeazzi, M.
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Astrophysics - Abstract
The number of detected baryons in the Universe at z<0.5 is much smaller than predicted by standard big bang nucleosynthesis and by the detailed observation of the Lyman alpha forest at red-shift z=2. Hydrodynamical simulations indicate that a large fraction of the baryons today is expected to be in a ``warm-hot'' (10^5-10^7K) filamentary gas, distributed in the intergalactic medium. This gas, if it exists, should be observable only in the soft X-ray and UV bands. Using the predictions of a particular hydrodynamic model, we simulated the expected X-ray flux as a function of energy in the 0.1-2 keV band due to the Warm-Hot Intergalactic Medium (WHIM), and compared it with the flux from local and high red-shift diffuse components. Our results show that as much as 20% of the total diffuse X-ray background (DXB) in the energy range 0.37-0.925keV could be due to X-ray flux from the WHIM, 70% of which comes from filaments at redshift z between 0.1 and 0.6. Simulations done using a FOV of 3', comparable with that of Suzaku and Constellation-X, show that in more than 20% of the observations we expect the WHIM flux to contribute to more than 20% of the DXB. These simulations also show that in about 10% of all the observations a single bright filament in the FOV accounts, alone, for more than 20% of the DXB flux. Red-shifted oxygen lines should be clearly visible in these observations., Comment: 19 pages, 6 figures
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- 2006
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24. Two Models for Bolometer and Microcalorimeter Detectors with Complex Thermal Architectures
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Appel, J. W. and Galeazzi, M.
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Physics - Instrumentation and Detectors ,Astrophysics - Abstract
We have developed two analytical models to describe the performance of cryogenic microcalorimeters and bolometers. One of the models is suitable to describe Transition Edge Sensor (TES) detectors with an integrated absorber, the other is suitable for detectors with large absorbers. Both models take into account hot-electron decoupling and absorber decoupling. The differential equations describing these models have been solved using block diagram algebra. Each model has produced closed form solutions for the detector's responsivity, dynamic impedance, and noise equivalent power for phonon noise, Johnson noise, amplifier noise, 1/f noise, and load resistor noise., Comment: 11 pages, 7 figures, 1 Table
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- 2005
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25. A Microcalorimeter and Bolometer Model
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Galeazzi, M. and McCammon, D.
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Astrophysics ,Physics - Instrumentation and Detectors - Abstract
The standard non-equilibrium theory of noise in ideal bolometers and microcalorimeters fails to predict the performance of real devices due to additional effects that become important at low temperature. In this paper we extend the theory to include the most important of these effects, and find that the performance of microcalorimeters operating at 60 mK can be quantitatively predicted. We give a simple method for doing the necessary calculations, borrowing the block diagram formalism from electronic control theory., Comment: 20 pages, 15 figures
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- 2003
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26. A High Spectral Resolution Observation of the Soft X-ray Diffuse Background with Thermal Detectors
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McCammon, D., Almy, R., Apodaca, E., Tiest, W. Bergmann, Cui, W., Deiker, S., Galeazzi, M., Juda, M., Lesser, A., Mihara, T., Morgenthaler, J. P., Sanders, W. T., Zhang, J., Figueroa-Feliciano, E., Kelley, R. L., Moseley, S. H., Mushotzky, R. F., Porter, F. S., Stahle, C. K., and Szymkowiak, A. E.
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Astrophysics - Abstract
A high spectral resolution observation of the diffuse X-ray background in the 60 - 1000 eV energy range has been made using an array of thirty-six 1 mm^2 micro-calorimeters flown on a sounding rocket. Detector energy resolution ranged from 5-12 eV FWHM, and a composite spectrum of ~ 1 steradian of the background centered at l = 90, b = +60 was obtained with a net resolution of ~ 9 eV. The target area includes bright 1/4 keV regions, but avoids Loop I and the North Polar Spur. Lines of C VI, O VII, and O VIII are clearly detected with intensities of 5.4 +/- 2.3, 4.8 +/- 0.8, and 1.6 +/- 0.4 photons cm^-2 s^-1 sr^-1, respectively. The oxygen lines alone account for a majority of the diffuse background observed in the ROSAT R4 band that is not due to resolved extragalactic discrete sources. We also have a positive detection of the Fe-M line complex near 70 eV at an intensity consistent with previous upper limits that indicate substantial gas phase depletion of iron. We include a detailed description of the instrument and its detectors., Comment: To appear in The Astrophysical Journal
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- 2002
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27. P264 THE RELATIONSHIP BETWEEN MEAN DAILY HEART RATE AND THE INCIDENCE OF CARDIAC ARRHYTHMIAS IN PATIENTS WITH WEARABLE CARDIAC DEFIBRILLATOR
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Matteucci, A, primary, Pignalberi, C, additional, Pandozi, C, additional, Magris, B, additional, Meo, A, additional, Schiaffini, G, additional, Russo, M, additional, Galeazzi, M, additional, Mocini, D, additional, Aquilani, S, additional, and Colivicchi, F, additional
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- 2023
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28. C69 SHORT–TERM OUTCOMES OF ABLATION INDEX–GUIDED CAVOTRICUSPID ISTHMUS ABLATION VERSUS UNIPOLAR RECORDED POTENTIAL INVERSION: A RANDOMIZED, SINGLE–CENTRE STUDY
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Matteucci, A, primary, Galeazzi, M, additional, Russo, M, additional, Schiaffini, G, additional, Cappuccio, C, additional, Di Fusco, S, additional, Lombardi, E, additional, Pandozi, C, additional, and Colivicchi, F, additional
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- 2023
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29. C55 A GIANT PSEUDOANEURYSM OF MITRAL–AORTIC INTERVALVULAR FIBROSA PRESENTING AS RECENT–ONSET ANGINA AND CARDIAC ARREST DUE TO VENTRICULAR FIBRILLATION
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Tofoni, P, primary, Patani, F, additional, Vagnarelli, F, additional, Lofiego, C, additional, Capodaglio, I, additional, Dottori, M, additional, Angelini, L, additional, Francioni, M, additional, Bonanni, C, additional, Grossi, P, additional, Galeazzi, M, additional, D‘Alfonso, A, additional, Marini, M, additional, Di Eusanio, M, additional, and Perna, G, additional
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- 2023
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30. P101 HIGH–DENSITY MAPPING OF KOCH‘S TRIANGLE DURING SINUS RHYTHM AND TYPICAL AV NODAL REENTRANT TACHYCARDIA INTEGRATED WITH THE DIRECT RECORDING OF ATRIOVENTRICULAR NODE STRUCTURES POTENTIAL: A MULTICENTER NON–RANDOMIZED STUDY
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Matteucci, A, primary, Russo, M, additional, Galeazzi, M, additional, Botto, G, additional, Castro, A, additional, Zingarini, G, additional, Del Giorno, G, additional, Papa, A, additional, Di Belardino, N, additional, Segreti, L, additional, Pepi, P, additional, Casale, M, additional, Treglia, S, additional, Nicolis, D, additional, Carbone, A, additional, Lavalle, C, additional, Malacrida, M, additional, Pandozi, C, additional, and Colivicchi, F, additional
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- 2023
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31. P296 WHAT IF CARDIAC SURGEONS PERFORM TRANS–CATHETER AORTIC VALVE INTERVENTIONS?
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Malvindi, P, primary, Berretta, P, additional, Capestro, F, additional, Galeazzi, M, additional, Bifulco, O, additional, Alfonsi, J, additional, Cefarelli, M, additional, Zingaro, C, additional, Pierri, M, additional, D‘Alfonso, A, additional, and Di Eusanio, M, additional
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- 2023
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32. P291 BUILDING UP A TRANSFEMORAL TAVI PROGRAM DONE BY CARDIAC SURGEONS: OUR EXPERIENCE IN 502 PATIENTS
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Berretta, P, primary, Capeestro, F, additional, Galeazzi, M, additional, Bifulco, O, additional, Alfonsi, J, additional, Buratto, B, additional, Cefarelli, M, additional, Malvindi, P, additional, and Di Eusanio, M, additional
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- 2023
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33. P102 DIFFERENCES IN HIGH–DENSITY MAPPING OF KOCH‘S TRIANGLE DURING TYPICAL AV NODAL REENTRANT TACHYCARDIA INTEGRATED AND NOT INTEGRATED WITH DIRECT RECORDING OF ATRIOVENTRICULAR NODE STRUCTURES POTENTIAL: A MULTICENTER NON–RANDOMIZED STUDY
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Matteucci, A, primary, Galeazzi, M, additional, Russo, M, additional, Botto, G, additional, Castro, A, additional, Zingarini, G, additional, Del Giorno, G, additional, Papa, A, additional, Di Belardino, N, additional, Segreti, L, additional, Pepi, P, additional, Nicolis, D, additional, Carbone, A, additional, Lavalle, C, additional, Casale, M, additional, Treglia, S, additional, Malacrida, M, additional, Pandozi, C, additional, and Colivicchi, F, additional
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- 2023
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34. Real-world experience of tocilizumab in rheumatoid arthritis: sub-analysis of data from the Italian biologics’ register GISEA
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Iannone, F., Ferraccioli, G., Sinigaglia, L., Favalli, E. G., Sarzi-Puttini, P., Atzeni, F., Gorla, R., Bazzani, C., Govoni, M., Farina, I., Gremese, E., Carletto, A., Giollo, A., Galeazzi, M., Foti, R., Bianchino, L., La Grasta, L., and Lapadula, G.
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- 2017
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35. Can balneotherapy modify microRNA expression levels in osteoarthritis? A comparative study in patients with knee osteoarthritis
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Giannitti, C., De Palma, A., Pascarelli, N. A., Cheleschi, S., Giordano, N., Galeazzi, M., and Fioravanti, Antonella
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- 2017
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36. Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals
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Sibeck, David G, Allen, R, Aryan, H, Bodewits, D, Brandt, P, Branduardi-Raymont, G, Brown, G, Carter, J. A, Collado-Vega, Y. M, Collier, M. R, Connor, H. K, Cravens, T. E, Ezoe, Y, Fok, M.-C, Galeazzi, M, Gutynska, O, Holmström, M, Hsieh, S.-Y, Ishikawa, K, Koutroumpa, D, Kuntz, K. D, Leutenegger, M, Miyoshi, Y, Porter, F. S, Purucker, M. E, Read, A. M, Raeder, J, Robertson, I. P, Samsonov, A. A, Sembay, S, Snowden, S. L, Thomas, N. E, von Steiger, R, Walsh, B. M, and Wing, S
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Astrophysics - Abstract
Both heliophysics and planetary physics seek to understand the complex nature of the solar wind's interaction with solar system obstacles like Earth's magnetosphere, the ionospheres of Venus and Mars, and comets. Studies with this objective are frequently conducted with the help of single or multipoint in situ electromagnetic field and particle observations, guided by the predictions of both local and global numerical simulations, and placed in context by observations from far and extreme ultraviolet (FUV, EUV), hard X-ray, and energetic neutral atom imagers (ENA). Each proposed interaction mechanism (e.g., steady or transient magnetic reconnection, local or global magnetic reconnection, ion pick-up, or the Kelvin- Helmholtz instability) generates diagnostic plasma density structures. The significance of each mechanism to the overall interaction (as measured in terms of atmospheric/ionospheric loss at comets, Venus, and Mars or global magnetospheric/ionospheric convection at Earth) remains to be determined but can be evaluated on the basis of how often the density signatures that it generates are observed as a function of solar wind conditions. This paper reviews efforts to image the diagnostic plasma density structures in the soft (low energy, 0.1-2.0 keV) X-rays produced when high charge state solar wind ions exchange electrons with the exospheric neutrals surrounding solar system obstacles.
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- 2018
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37. High-definition electro-anatomical mapping of Koch’s Triangle including AV node potentials recordings in consecutive AVNRT patients
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Pandozi, C, primary, Botto, GL, additional, Del Giorno, G, additional, Papa, AA, additional, Castro, A, additional, Di Belardino, N, additional, Viani, S, additional, Russo, M, additional, Brasca, F, additional, Carbone, A, additional, Galeazzi, M, additional, Casale, MC, additional, Treglia, S, additional, Malacrida, M, additional, and Colivicchi, F, additional
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- 2022
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38. C13 COMPARISON OF MINIMALLY INVASIVE VERSUS CONVENTIONAL THORACIC AORTIC OPERATIONS: EARLY AND MID–TERM RESULTS IN A SERIES OF 624 PATIENTS
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Berretta, P, primary, Galeazzi, M, additional, Chiuselli, G, additional, Codecasa, R, additional, Alfonsi, J, additional, Braconi, L, additional, Rapisarda, F, additional, Bonacchi, M, additional, Malvindi, P, additional, Stefano, P, additional, and Di Eusanio, M, additional
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- 2022
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39. C17 SIMPLIFIED MINIMALLY INVASIVE MITRAL VALVE SURGERY THROUGH A DIRECT VISION TRANSAXILLARY APPROACH: PROCEDURAL AND 30–DAYS OUTCOMES
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Malvindi, P, primary, Berretta, P, additional, Alfonsi, J, additional, Galeazzi, M, additional, Bifulco, O, additional, Capestro, F, additional, Zingaro, C, additional, and Di Eusanio, M, additional
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- 2022
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40. Understanding Factors Associated With Psychomotor Subtypes of Delirium in Older Inpatients With Dementia
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Morandi, A, Zambon, A, Di Santo SG, Mazzone, A, Cherubini, A, Mossello, E, Bo, M, Marengoni, A, Bellelli, G, Rispoli, V, Malara, A, Spadea, F, Di Cello, S, Ceravolo, F, Fabiano, F, Chiaradia, G, Amedeo, G, Peluso, L, Taristano, A, Settembrini, V, Capomolla, D, Citrino, A, Scriva, A, Bruno, I, Secchi, R, De Martino, E, Muccinelli, R, Lupi, G, Paonessa, P, Fabbri, A, Passuti, Mt, Castellari, S, Po, A, Gaggioli, G, Varesi, M, Moneti, P, Capurso, S, Latini, V, Ghidotti, S, Riccardelli, F, Macchi, M, Rigo, R, Pascale, C, Bosio, A, Cerrato, F, Bardelli, B, Boffelli, S, Cassinadri, A, Franzoni, S, Spazzini, E, Andretto, D, Tonini, G, Andreani, L, Coralli, M, Balotta, A, Cancelliere, R, Ballardini, G, Simoncelli, M, Mancini, A, Strazzacapa, M, Cavallino, P, Fabio, S, De Filippi, F, Giudice, C, Floris, P, D’Elia, K, Dentizzi, C, Azzini, M, Cazzadori, M, Mastroeni, V, Bertassello, P, Santana, H, Benati, C, Nesta, E, Tobaldini, C, Antonioli, A, Guerini, F, Tambare, E, Mombelloni, P, Fontanini, F, Lassa, G, Pizzorni, C, Oliverio, M, Del Grosso LL, Giavedoni, C, Bidoli, G, Mazzei, B, Corsonello, A, Fusco, S, Vena, S, De Vuono, T, Maiuri, G, Fimognari, Fl, Arone, A, Sgrò, G, Nicolazzo, R, Castegnaro, E, De Rosa, S, Bazzano Sechi, R, Benvenuti, E, Del Lungo, I, Giardini, S, Giulietti, C, Di Bari, M, Barghini, E, Paoli, M, Fiordelli, I, Barucci, R, Sgrilli, F, Bertoletti, E, D'Amico, F, Caronzolo, F, Grippa, A, Lombardo, G, Pipicella, T, Satta, A, Corica, F, Prestipino, Gv, Larosa, D, Cucinotta, D, Basile, G, March, A, Nitti, Mt, Felici, A, Pavan, S, Piazzani, F, Lunelli, A, Dimori, S, Margotta, A, Soglia, T, Postacchini, D, Brunelli, R, Santini, S, Francavilla, M, Macchiati, I, Sorvillo, F, Giuli, C, Mecocci, P, Longo, A, Conestabile della Staffa, M, Perticone, F, Addesi, D, Cella Rosa, P, Bencardino, G, Falbo, T, Grillo, N, Marco, F, Mirella, F, Fantò, F, Isaia, G, Pezzilli, S, Bergamo, D, Furno, E, Rrodhe, S, Lucarini, S, Dijk, B, Dall'Acqua, F, Cappelletto, F, Calvani, D, 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Suigo, G, Faverio, P, Gori, A, Perego, S, Zanasi, M, Moniello, G, Rostagno, C, Cartei, A, Polidori, G, Ungar, A, Melis, Mr, Martellini, E, Torrini, M, Giordano, A, Leone, G, Migliorini, M, Caramelli, F, Battiston, B, Berardino, M, Cavallo, S, Massè, A, Santoro, A, Lombardi, B, D'Ippolito, P, Furini, A, Villani, D, Raimondi, C, Guarneri, M, Paolucci, S, Bassi, A, Coiro, P, De Angelis, D, Morone, G, Venturiero, V, Palleschi, L, Raganato, P, Di Niro, G, Rosa, Ca, Bove, L, Imoscopi, A, Tibaldi, V, Calvi, E, Clementi, C, Zanocchi, M, Agosta, L, Crasia, A, Spertino, A, Nortarelli, A, Provenzano, G, Principato, P, Criasia, A, Spertino, E, Mari, D, Romano, Fy, Rosini, F, Mansi, M, Rossi, S, Riccardelli, A, Inzaghi, L, Bonini, G, Rossi, P, Potena, A, Lichii, M, Candiani, T, Grimaldi, W, Bertani, E, Porta, A, Calogero, P, Pinto, D, Bernardi, R, Nicolino, F, Galetti, C, Gianstefani, A, Corvalli, G, Mulazzani, L, Odetti, P, Monacelli, F, Prefumo, M, Canepa, M, Minaglia, C, Paolisso, G, Rizzo, Mr, 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L, Tesi, F, Martella, L, Imbrici, R, Guerrini, G, Scotuzzi, Am, Sozzi, F, Valenti, L, Chiarello, A, Monella, M, Pilotto, A, Prete, C, Senesi, B, Meta, Ac, Pendenza, E, Pasqualetti, G, Polini, A, Tognini, S, Ballino, E, Dell'Aquila, G, Gasparrini, Pm, Marotti, E, Migale, M, Scrimieri, A, Falsetti, L, Toigo, G, Ceschia, G, Rosso, A, Tongiorgi, C, Scarpa, C, Pacchioni, M, De Dominicis, L, Pucci, E, Renzi, S, Cartechini, E, Tomassini, Pf, Del Gobbo, M, Ugenti, F, Romeo, P, Nardelli, A, Lauretani, F, Visioli, S, Montanari, I, Ermini, F, Pigato, G, Simeone, E, Colameco, F, Cecamore, A, Scurti, R, Lupinetti, Mc, Barbujani, M, Giampieri, M, Amoruso, R, Piccinini, M, Ferrari, C, Gambetti, C, Sfrappini, M, Semeraro, L, Striuli, R, Pelliccioni, G, Marinelli, D, Fabi, K, Rossi, T, Pesallaccia, M, Sabbatini, D, Gobbi, B, Cerqua, R, Tagliani, G, Schlauser, E, Caser, L, Caramello, E, Sandigliano, F, Rosso, G, Ferrari, A, Bendini, C, Davoli, Ml, Casella, M, Prampolini, R, Scevola, M, Vitale, E, Brugiolo, V, Fagherazzi, C, Scarpa, A, Zara, D, Bertozzo, G, Granziera, S, Berazzuol, M, Maugeri, D, Sorace, R, Anzaldi, M, De Gesu, R, Morrone, G, Davolio, F, Fabbo, A, Palmieri, M, Zoli, M, Forti, P, Pirazzoli, L, Fabbri, E, Terenzi, L, Bergolari, F, Wenter, C, Ruffini, I, Insam, M, Abraham, E, Kirchlechner, C, Antonino, L, Grazia, Am, Parise, P, Boccali, A, Amici, S, Gambacorta, M, Lasagni, A, Lovati, R, Giovinazzo, F, Kimak, E, Zappa, P, Medici, F, Lo Castro, M, Mauro, F, De Luca, A, Sancesario, G, Martorana, A, Scaricamazza, B, Di Lorenzo, F, Liguori, C, Lasco, A, Vita, N, Giomi, M, Forte, F, Padovani, A, Rozzini, L, Caratozzolo, S, Cottino, M, Vitali, S, Marelli, E, Tripi, G, Miceli, S, Urso, G, Grioni, G, Vezzadini, G, Misaggi, G, Forlani, C, Avanzi, S, Saulle, S, Casarini, C, Viggiano, M, Alberto, L, Ghianda, D, Iemolo, F, Sanzaro, E, D'Asta, G, Proietto, M, Carnemolla, A, Razza, G, Spadaro, D, Bertolotti, M, Mussi, C, Neviani, F, Chiesa, R, Guerzoni, V, Morselli, L, 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Sabatini, T, Mussio, E, Magni, E, Bianchetti, A, Crucitti, A, Titoldini, G, Cossu, B, Fascendini, S, Licini, C, Tomasoni, A, Calderazzo, M, Tropiano, D, Luganà, V, Melotti, Rm, Lilli, A, Buda, S, Adversi, M, Noro, G, Turco, R, Ubezio, Mc, Mantovani, Ar, Viola, Mc, Serrati, C, Pretta, S, Infante, M, Gentile, S, D'Ambrosio, V, Mazzanti, P, Brambilla, C, Sportelli, S, Platto, C, Faraci, B, Quattrocchi, D, Pisu, C, Sicuro, F, Zagnoni, P, Ghiglia, S, Mosca, M, Corazzin, I, Deola, M, Biagini, Ca, Bencini, F, Cantini, C, Tonon, E, Pierinelli, S, Onofrj, M, Thomas, A, Filomena, B, Bonanni, L, Cacchiò, G, Comi, G, Magnani, G, Santangelo, R, Mazzeo, S, Caso, F, Cecchetti, G, Sant’Angelo, R, Barbieri, C, Giroldi, L, Bandini, F, Masina, M, Malservisi, S, Cicognani, A, Ricca, L, Piccininni, M, Tassinari, T, Brogi, D, Sugo, A, Filippi, A, Manfredi, S, Vanni, V, Usai, Ca, Colombo, E, Renna, Fv, Sanchella, A, Prete, M, Bisagni, P, Masini, R, Carrabetta, S, Barone, A, Razzano, M, Imperoli, G, Bini, A, Serra, F, D’Agostino, V, Gianolla, F, Pietrangeli, L, Velardi, A, Di Cello, E, Rosati, C, Casali, N, Sessa, M, Abruzzi, L, Costanzi, C, Bini, P, Pignata, M, Bonagurio, E, Vollery, M, Carrieri, G, Cioni, G, Toschi, A, Metra, M, Ranieri, P, Zucchelli, A, Ceccon, A, Magrin, L, Marin, S, Barbara, S, Ghedini, L, Moroni, M, Pitagora, M, Pallotti, Mc, Gottardi, F, Tomasoni, C, Cappuccio, M, Guerini, S, Guerini, V, Merla, L, Tovaglieri, M, Bongiorni, N, Grillo, A, Arenare, F, Tonino, M, Kanah, D, Vianello, Pg, Balducci, U, Sidoti, V, Montanari, S, Murelli, T, Busonera, F, Albanese, P, Maselli, M, Bolzetta, F, Fabris, R, Durante Mangoni, E, Testoni, M, Di Stefano, F, Seccia, L, Morabito, D, Sonzina, V, Fabiano, M, Di Giorgio Annabella, De Cosmo Salvatore, Greco, A, D’Onofrio, G, Sancarlo, D, Resta, G, Girardello, R, Minervini, S, Boni, M, Vitali, Mg, Pizzoni, M, De Colle, P, Frattola, A, Orlandini, F, La Regina, M, Filice, M, Padulo, F, Margheriti, C, Rolano, D, Sacchelli, C, Moscatelli, G, Radaelli, G, Montini, E, Novello, M, Bramuzzo, I, Bertin, N, Rinaldo, E, Paolillo, C, Riccardi, A, Benedetti, C, Ricci, B, Montagna, F, Cutaia, C, Baca, O, Colombo, M, Procino, G, Tararà, R, Dell’Acqua, D, Cislaghi, S, Cairati, M, Porta, M, Scaglione, L, De Feo, M, Vertolli, P, Salvati, L, Cinotti, S, De Santis, V, Biferi, E, Cheli, P, Rebizzo, R, Minisola, S, Colangelo, L, Abete, P, Liguori, I, Curcio, F, Spassini, G, Engheben, M, Rotunno, S, Arosio, P, Angelini, C, Reggiani, F, Cappelli, A, Marcheselli, S, Fratticci, L, Ranzani, P, Cesarini, S, Cerini, A, Generoso, U, Gallucci, F, Serra, E, Sola, M, Delitala, A, Pes, C, Lobianco, G, Giani, A, Famularo, S, Sandini, M, Pinotti, E, Gianotti, L, Alessandro, D, Chiara, P, Giulia, L, Alessandro, G, Giannotti, L, Battuello, A, Pintore, G, Rossi, A, Rubele, S, Sant, S, Vignati, M, Clerici, D, Rosa, F, Bandirali, Mp, Cattaneo, N, Boffi, L, Avalli, L, Scanziani, M, De Notaris, S, Del Santo, P, Catalano, F, Fogli, D, Di Bella, G, Landi, F, Salini, S, Brunetti, Ma, Cappa, G, Galvagno, G, Cena, P, Gerardo, B, Raspo, S, Pedrotti, S, Palmieri, Vo, Palasciano, G, Belfiore, A, Portincasa, P, Sabbà, C, Solfrizzi, V, D’Introno, A, Valiani, V, Bologna, C, Ciarambino, T, Turelli, P, Pazzaglia, U, Rodella, F, Piana, G, Castellano, M, Garelli, A, Casella, E, Campana, F, Coschignano, Ma, Marinangeli, L, Lorico, F, Bazzano, S, Menculini, G, Gelosa, G, Ambrogio, Tv, Piras, V, Ciricugno, A, Bollari, A, Coen, D, Magliola, R, Milanesio, D, Muzzulini, Cl, Fogliacco, P, Turla, M, Cotelli, Ms, Bianchi, M, Siano, P, Capo, G, Napoletano, R, Politi, C, Mancini, C, Del Buono, C, De Bartolomeo, G, Martinelli, A, Cefalogli, C, Cozzi, R, Virtuani, Ag, Moschettini, G, Mastroianni, F, Roglia, D, D’Amico, G, Palella, M, Endrizzi, C, Trotta, L, Zanetti, O, Terazzi, E, Sacchetti, M, Fleetwood, T, Tondo, G, Di Fazio, I, Orsitto, G, Fabbro, E, D’Imporzano, E, Casanova, A, Bertolio, S, Nervo, E, Silvestri, R, Semproni, E, Pintus, M, Aloe, F, Tagliaccica, A., Morandi A., Zambon A., Di Santo S.G., Mazzone A., Cherubini A., Mossello E., Bo M., Marengoni A., Piccoli T., Bellelli G., Rispoli V., Malara A., Spadea F., Di Cello S., Ceravolo F., Fabiano F., Chiaradia G., Gabriele A., Lenino P., Andrea T., Settembrini V., Capomolla D., Citrino A., Scriva A., Bruno I., Secchi R., De Martino E., Muccinelli R., Lupi G., Paonessa P., Fabbri A., Passuti M.T., Castellari S., Po A., Gaggioli G., Varesi M., Moneti P., Capurso S., Latini V., Ghidotti S., Riccardelli F., Macchi M., Rigo R., Claudio P., Angelo B., Flavio C., Benedetta B., Boffelli S., Cassinadri A., Franzoni S., Spazzini E., Andretto D., Tonini G., Andreani L., Coralli M., Balotta A., Cancelliere R., Ballardini G., Simoncelli M., Mancini A., Strazzacapa M., Fabio S., De Filippi F., Giudice C., Dentizzi C., Azzini M., Cazzadori M., Mastroeni V., Bertassello P., Claudia Benati H.S., Nesta E., Tobaldini C., Guerini F., Elena T., Mombelloni P., Fontanini F., Gabriella L., Pizzorni C., Oliverio M., Del Grosso L.L., Giavedoni C., Bidoli G., Mazzei B., Corsonello A., Fusco S., Vena S., De Vuono T., Maiuri G., Luca F.F., Andrea A., Giovanni S., Rossella N., Castegnaro E., De Rosa S., Sechi R.B., Benvenuti E., Del Lungo I., Giardini S., Giulietti C., Mauro D.B., Eleonora B., Martina P., Irene F., Riccardo B., Federica S., Ilaria D.L., Bertoletti E., D'Amico F., Caronzolo F., Grippa A., Lombardo G., Pipicella T., Antonino S., Francesco C., Valeria P.G., Daniela L., Domenico C., Giorgio B., March A., Nitti M.T., Felici A., Pavan S., Piazzani F., Lunelli A., Dimori S., Margotta A., Soglia T., Postacchini D., Brunelli R., Santini S., Francavilla M., Macchiati I., Sorvillo F., Giuli C., Mecocci P., Longo A., Perticone F., Addesi D., Rosa P.C., Bencardino G., Falbo T., Grillo N., Marco F., Mirella F., Fanto F., Isaia G., Pezzilli S., Bergamo D., Furno E., Rrodhe S., Lucarini S., Dijk B., Dall'Acqua F., Cappelletto F., Calvani D., Becheri D., Giuseppe M., Costanza M., Vito A., Francesca B., Magherini L., Novella M., Franca B., Lucia Gambardella P.M., Valente C., Ilaria B., Alice F., Porrino P., Ceci G., Giuliana B., Michela T., Eleonora C., Ettore E., Camellini C., Servello A., Grassi A., Rozzini R., Tironi S., Grassi M.G., Troisi E., Carlo C., Simona Gabriella D.S., Flaminia F., Federica R., Beatrice P., Sofia T., Gabutto A., Quazzo L., Rosatello A., Suraci D., Tagliabue B., Perrone C., Ferrara L., Castagna A., Tremolada M.L., Giuseppe C., Stefano B., Davide O., Piano S., Serviddio G., Lo Buglio A., Gurrera T., Merlo V., Rovai C., Cotroneo A.M., Carlucci R., Abbaldo A., Monzani F., Qasem A.A., Bini G., Tafuto S., Galli G., Bruni A.C., Mancuso G., Calipari D., Giuseppe Massimiliano D.L., Bernardini B., Corsini C., Michele C., Sara D.F., Cagnin A., Fragiacomo F., Pompanin S., Piero A., Marco C., Zurlo A., Guerra G., Pala M., Menozzi L., Gatti C.D., Magon S., Roberto M., Alfredo D.G., Fabio F., Ruana T., Elisa M., Christian M., Marco P., Massimo G., Di Francesco V., Faccioli S., Pellizzari L., Giorgia F., Barbagallo G., Lunardelli M.L., Martini E., Ferrari E., Macchiarulo M., Corneli M., Bacci M., Battaglia G., Anastasio L., Lo Storto M.S., Seresin C., Simonato M., Loreggian M., Cestonaro F., Durando M., Latella R., Mazzoleni M., Russo G., Ponte M., Valchera A., Salustri G., Petritola D., Costa A., Sinforiani E., Cotta M.R., Pizio R.N., Cester A., Formilan M., Pietro B., Carbone P., Cazzaniga I., Appollonio I., Cereda D., Stabile A., Xhani R., Acampora R., Tremolizzo L., Federico P., Antonio C., Valerio P., Cesare B., Zhirajr M., Giovanni V., Maria A., Mariaelena S., Bottacchi E., Bucciantini E., Di Giovanni M., Franchi F., Lucchetti L., Mariani C., Grande G., Rapazzini P., Marco M., Romanelli G., Franco N., Alessio M., Nicola L., Laura P., Nazario P., Chiara G., Soccorso P., Andrea S., Luca B., Francesca S., Roberto A., Anna C., Fugazza L., Guerrini C., De Paduanis G., Iallonardo L., Palumbo P., Zuliani G., Ortolani B., Capatti E., Soavi C., Bianchi L., Francesconi D., Miselli A., Gloria B., Tommaso R., Chiara P., Agata M.M., Marco D.A., Luca M., Gianluca G., Suardi T., Zaccarini C., Manuela R., Mirra G., Muti E., Bottura R., Gianpaolo M., Secreto P., Bisio E., Cecchettani M., Naldi T., Pallavicino A., Pugliese M., Iozzo R.C., Grassi G., Michele B., Raffaella D.O., Fosca Q.T., Giorgio G.C., Giovanni P., Ernesto C., Mannironi A., Giorli E., Oberti S., Fierro B., Giacalone F., Mandas A., Serchisu L., Costaggiu D., Pinna E., Orru F., Mannai M., Cordioli Z., Pelizzari L., Turcato E., Arduini P., Cacace C., Chiloiro R., Cimino R., Ruberto C., Giovanni R., Pietro G., Laura G., Alberto C., Carmen R., Santo P.D., Andriolli A., Burattin G., Rossi L., Andreolli Antonino C.G., Tezza F., Maddalena P., Laura S., Crippa P., Aloisio P., Di Monda T., Malighetti A., Galbassini G., Salutis D., Ivaldi C., Russo A.M., Bennati E., Pino E., Zavarise G., Pesci A., Suigo G., Faverio P., Andrea G., Sabrina P., Zanasi M., Moniello G., Rostagno C., Cartei A., Polidori G., Ungar A., Melis M.R., Martellini E., Enrico M., Monica T., Antonella G., Giovanna L., Migliorini M., Caramelli F., Battiston B., Berardino M., Cavallo S., Alessandro M., Anna S., Lombardi B., D'Ippolito P., Furini A., Villani D., Clara R., Guarneri M., Paolucci S., Bassi A., Coiro P., De Angelis D., Morone G., Venturiero V., Palleschi L., Raganato P., Di Niro G., Rosa C.A., Loredana B., Imoscopi A., Tibaldi V., Bottignole G G., Calvi E., Clementi C., Zanocchi M., Agosta L., Nortarelli A., Provenzano G., Mari D., Romano F.Y., Rosini F., Mansi M., Rossi S., Geriatria A.R., Inzaghi L., Bonini G., Rossi P., Potena A., Lichii M., Candiani T., Grimaldi W., Bertani E., Alessandra P., Calogero P., Pinto D., Bernardi R., Nicolino F., Galetti C., Gianstefani A., Giulia C., Lorenzo M., Odetti P., Monacelli F., Prefumo M., Fiammetta M., Canepa M., Minaglia C., Paolisso G., Rizzo M.R., Prestano R., Dalise A.M., Barra D., Bosco L.D., Asprinio V., Dallape L., Perina E., Incalzi R.A., Bartoli I.R., Pluderi A., Maina A., Pecoraro E., Sciarra M., Prudente A., Paola M., Francesca M., Manuel V., Luisella C., Maria P.L., Tina S., Benini L., Levato F., Mhiuta V., Alius F., Davidoaia D., Giardini V., Garancini M., Bellamoli C., Terranova L., Bozzini C., Tosoni P., Provoli E., Cascone L., Dioli A., Ferrarin G., Bucci A., Bua G., Fenu S., Bianchi G., Casella S., Romano V., Maurizio P., Mascherona I., Belotti G., Cavaliere S., Cuni E., Merciuc N., Oberti R., Veneziani S., Capoferri E., De Bernardi E., Colombo K., Bravi M., Nicoletta N., D'Arcangelo P., Montenegro N., Montanari R., Lamanna P., Gasperini B., Isabella M., Stefania D., Gaia A., Filippo C., Palama C., Di Emidio C., Scarpini E., Arighi A., Fumagalli G., Basilico P., De Amicis Margherita M., Marta M., Diletta M., Granata A., Ranalli C., Cammilli A., Cavallini M.C., Tricca M., Natella D., Gabbani L., Tesi F., Martella L., Imbrici R., Guerrini G., Scotuzzi A.M., Sozzi F., Valenti L., Chiarello A., Monia M., Pilotto A., Prete C., Senesi B., Meta A.C., Pendenza E., Pasqualetti G., Polini A., Tognini S., Ballino E., Dell'Aquila G., Gasparrini P.M., Marotti E., Migale M., Scrimieri A., Falsetti L., Salvi A., Toigo G., Ceschia G., Rosso A., Tongiorgi C., Scarpa C., De Dominicis L., Pucci E., Renzi S., Cartechini E., Tomassini P.F., Del Gobbo M., Ugenti F., Romeo P., Nardelli A., Lauretani F., Visioli S., Montanari I., Ermini F., Giordano A., Pigato G., Simeone E., Barbujani M., Giampieri M., Amoruso R., Piccinini M., Ferrari C., Gambetti C., Sfrappini M., Semeraro L., Striuli R., Pelliccioni G., Marinelli D., Fabi K., Rossi T., Pesallaccia M., Sabbatini D., Gobbi B., Cerqua R., Tagliani G., Schlauser E., Caser L., Caramello E., Sandigliano F., Rosso G., Ferrari A., Bendini C., Luisa D.M., Casella M., Prampolini R., Scevola M., Vitale E., Roberto B., Carlo F., Sergio F., Alberto S., Daniela Z., Giulia B., Serena G., Maugeri D., Sorace R., Anzaldi M., De Gesu R., Morrone G., Davolio F., Fabbo A., Palmieri M., Zoli M., Forti P., Pirazzoli L., Fabbri E., Terenzi L., Bergolari F., Wenter C., Ruffini I., Insam M., Abraham E., Kirchlechner C., Cucinotta D., Antonino L., Basile G., Grazia A.M., Parise P., Boccali A., Amici S., Gambacorta M., Lasagni A., Lovati R., Giovinazzo F., Kimak E., Zappa P., Medici F., Lo Castro M., Mauro F., De Luca A., Sancesario G., Martorana A., Scaricamazza B., Toniolo S., Di Lorenzo F., Liguori C., Lasco A., Vita N., Giomi M., Forte F., Padovani A., Rozzini L., Ceraso A., Salvatore C., Cottino M., Vitali S., Marelli E., Tripi G., Miceli S., Urso G., Grioni G., Vezzadini G., Misaggi G., Forlani C., Avanzi S., Serena S., Claudia C., Marilena V., Alberto L., Diego G., Alessandro G., Iemolo F., Sanzaro E., D'Asta G., Proietto M., Carnemolla A., Razza G., Spadaro D., Bertolotti M., Mussi C., Neviani F., Roberto C., Valentina G., Linda M., Francesca V., Tarozzi A., Balestri F., Mannarino G., Bigolari M., Natale A., Grassi S., Bottaro C., Stefanelli S., Bovone U., Tortorolo U., Quadri R., Leone G., Ponzetto M., Frasson P., Annoni G., Bruni A., Confalonieri R., Corsi M., Moretti D., Teruzzi F., Umidi S., Mazzola P., Perego S., Persico I., Olivieri G., Bonfanti A., Hajnalka S., Galeazzi M., Massariello F., Anzuini A., Caffarra P., Barocco F., Spallazzi M., Paolo C.G., Simonetta M., Chioatto P., Bortolamei S., Soattin L., Ruotolo G., Beneamino B., Giuseppe B., Bertazzoli M., Rota E., Adobati A., Scarpa A., Granziera S., Zuccher P., Fabbro A.D., Zara D., Lo Nigro A., Franchetti L., Toniolo M., Marcuzzo C., Rollone M., Guerriero F., Sgarlata C., Masse A., Zatti G., Piatti M., Graci J., Benati G., Boschi F., Biondi M., Fiumi N., Erika T., Locatelli S.M., Mauri S., Beretta M., Margheritis L., Desideri G., Liberatore E., Carucci A.C., Bonino P., Caput M., Antonietti M.P., Polistena G., De la Pierre F., Mari M., Massignani P., Tombesi F., Selvaggio F., Verbo B., Bodoni P., Marchionni N., Sabatini T., Mussio E., Magni E., Bianchetti A., Crucitti A., Titoldini G., Cossu B., Fascendini S., Licini C., Tomasoni A., Calderazzo M., Daniela T., Valentina L., Melotti R.M., Lilli A., Buda S., Adversi M., Noro G., Turco R., Ubezio M.C., Mantovani A.R., Viola M.C., Serrati C., Pretta S., Infante M., Gentile S., D'Ambrosio V., Mazzanti P., Brambilla C., Sportelli S., Platto C., Faraci B., Quattrocchi D., Pernigotti L.M., Pisu C., Sicuro F., Zagnoni P., Ghiglia S., Mosca M., Corazzin I., Deola M., Biagini C.A., Bencini F., Cantini C., Tonon E., Pierinelli S., Onofrj M., Thomas A., Filomena B., Bonanni L., Gabriella C., Comi G., Magnani G., Santangelo R., Mazzeo S., Francesca C., Giordano C., Roberto S.A., Barbieri C., Giroldi L., Bandini F., Masina M., Malservisi S., Cicognani A., Ricca L., Piccininni M., Tassinari T., Brogi D., Sugo A., Alessandra F., Sonia M., Valerio V., Andrea U.C., Enrico C., Vera R.F., Assunta S., Gianmaria Z., Mauro P., Barone A., Razzano M., Giuseppe I., Angela B., Francesco S., Valeria D.A., Federico G., Lucia P., Antonella V., Elisabetta D.C., Cristina R., Nadia C., Maria S., Luciano A., Chiara C., Bini P., Pignata M., Enrico B., Maria V., Giovanni C., Giorgio C., Piera R., Alberto Z., Ceccon A., Magrin L., Marin S., Barbara S., Matteo M., Caterina P.M., Carla R., Federica G., Clara T., Melania C., Giampaolo B., Stefano G., Valeria G., Lucia M., Giovambattista D., Ester L., Cecilia C.A., Maurizio T., Nadia B., Grillo A., Arenare F., Tonino M., David K., Giorgio V.P., Ubaldo B., Vincenzo S., Stefano M., Marino F., Busonera Flavio M.T., Paolo A., Monica M., Francesco B., Roberto F., Paolo B., DuranteMangoni E., Testoni M., Fabio D.S., Loredana S., Valeria S., Fabiano M., Annabella D.G., Salvatore D.C., Greco A., Grazia D.O., Daniele S., Gianluca R., Renzo G., Sergio M., Morena B., Vitali M., Marina P., Paolo D.C., Cristina S., Orlandini F., La Regina M., Desiree A., Mario B., Paola P., Padulo F., Cristina M., Dario R., Giancarla M., Guido R., Elena M., Marileda N., Igor B., Nicole B., Elena R., Paolillo C., Riccardi A., Claudia B., Barbara R., Silvia V., Oliver B., Mauro C., Eleonora M., Giuseppe P., Rosaria T., Maria C., Davide D.A., Stefania C., Massimo P., Luca S., Martina D.F., Paola V., Lia S., Sandro C., Valentina D.S., Erminia B., Paola C., Romina R., Minisola S., Luciano C., Pasquale A., Ilaria L., Guglielmo S., Marco E., Sara R., Paola A., Claudio A., Francesco R., Alessandro C., Simona M., Lara F., Paola R., Simonetta C., Antonella C., Generoso U., Fernando G., Giuliano C., Emanuela S., Mariolina S., Alessandro D., Giulia L., Famularo S., Sandini M., Pinotti E., Gianotti L., Antonella B., Giulia P., Sante G., Rossi A., Rubele S., Sant S., Marco V., Danila C., Fabio R., Bandirali M.P., Nicoletta C., Laura B., Paolo T., Luciano T., Leonello A., Margherita S., Stefania D.N., Pierluigi D.S., Laura R., Fabiana T., Giovanna C., Antonino A., Felice C., Danilo F., Giovanna D.B., Francesco L., Salini S., Angela B.M., Giorgetta C., Giovanni G., Gerardo B., Silvio R., Letizia S., Davide B., Rosaria R.M., Maria D.A., Raffaele P., Palmieri V.O., Palasciano G., Belfiore A., Portincasa P., Carlo S., Alessia D., Valiani V., Carolina B., Tiziana C., Paola T., Ugo P., Giacomo P., Castellano M., Anna G., Elisa C., Federica C., Antonietta C.M., Luigi M., Fabio L., Salvatore B., Gelosa G., Viviana A.T., Piras V., Andrea C., Alessandra B., Coen D., Magliola R., Milanesio D., Muzzulini C.L., Paolo F., Marinella T., Sofia C.M., Marta B., Siano P., Capo G., Napoletano R., Cecilia P., Mancini C., Del Buono C., De Bartolomeo G., Addolorata M., Carmen C., Giovanni V.A., Moschettini G., Franco M., Daniela R., D'Amico G., Mirella P., Endrizzi C., Trotta L., Ciarambino T., Orazio Z., Emanuela T., Marta S., Thomas F., Giacomo T., Ignazio D.F., Andrea B., Giuseppe O., Emanuela F., Serena A., Elena D.I., Serena B., Erika N., Roberto S., Elena S., Manuela P., Francesca A., Angelo T., Morandi, A, Zambon, A, Di Santo, S, Mazzone, A, Cherubini, A, Mossello, E, Bo, M, Marengoni, A, Bellelli, G, Rispoli, V, Malara, A, Spadea, F, Di Cello, S, Ceravolo, F, Fabiano, F, Chiaradia, G, Gabriele, A, Lenino, P, Andrea, T, Settembrini, V, Capomolla, D, Citrino, A, Scriva, A, Bruno, I, Secchi, R, De Martino, E, Muccinelli, R, Lupi, G, Paonessa, P, Fabbri, A, Passuti, M, Castellari, S, Po, A, Gaggioli, G, Varesi, M, Moneti, P, Capurso, S, Latini, V, Ghidotti, S, Riccardelli, F, Macchi, M, Rigo, R, Claudio, P, Angelo, B, Flavio, C, Benedetta, B, Boffelli, S, Cassinadri, A, Franzoni, S, Spazzini, E, Andretto, D, Tonini, G, Andreani, L, Coralli, M, Balotta, A, Cancelliere, R, Ballardini, G, Simoncelli, M, Mancini, A, Strazzacapa, M, Fabio, S, De Filippi, F, Giudice, C, Dentizzi, C, Azzini, M, Cazzadori, M, Mastroeni, V, Bertassello, P, Claudia Benati, H, Nesta, E, Tobaldini, C, Guerini, F, Elena, T, Mombelloni, P, Fontanini, F, Gabriella, L, Pizzorni, C, Oliverio, M, Del Grosso, L, Giavedoni, C, Bidoli, G, Mazzei, B, Corsonello, A, Fusco, S, 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Tina, S, Benini, L, Levato, F, Mhiuta, V, Alius, F, Davidoaia, D, Giardini, V, Garancini, M, Bellamoli, C, Terranova, L, Bozzini, C, Tosoni, P, Provoli, E, Cascone, L, Dioli, A, Ferrarin, G, Bucci, A, Bua, G, Fenu, S, Bianchi, G, Casella, S, Romano, V, Maurizio, P, Mascherona, I, Belotti, G, Cavaliere, S, Cuni, E, Merciuc, N, Oberti, R, Veneziani, S, Capoferri, E, De Bernardi, E, Colombo, K, Bravi, M, Nicoletta, N, D'Arcangelo, P, Montenegro, N, Montanari, R, Lamanna, P, Gasperini, B, Isabella, M, Stefania, D, Gaia, A, Filippo, C, Palama, C, Di Emidio, C, Scarpini, E, Arighi, A, Fumagalli, G, Basilico, P, De Amicis Margherita, M, Marta, M, Diletta, M, Granata, A, Ranalli, C, Cammilli, A, Cavallini, M, Tricca, M, Natella, D, Gabbani, L, Tesi, F, Martella, L, Imbrici, R, Guerrini, G, Scotuzzi, A, Sozzi, F, Valenti, L, Chiarello, A, Monia, M, Pilotto, A, Prete, C, Senesi, B, Meta, A, Pendenza, E, Pasqualetti, G, Polini, A, Tognini, S, Ballino, E, Dell'Aquila, G, Gasparrini, P, Marotti, E, Migale, M, Scrimieri, A, Falsetti, L, Salvi, A, Toigo, G, Ceschia, G, Rosso, A, Tongiorgi, C, Scarpa, C, De Dominicis, L, Pucci, E, Renzi, S, Cartechini, E, Tomassini, P, Del Gobbo, M, Ugenti, F, Romeo, P, Nardelli, A, Lauretani, F, Visioli, S, Montanari, I, Ermini, F, Giordano, A, Pigato, G, Simeone, E, Barbujani, M, Giampieri, M, Amoruso, R, Piccinini, M, Ferrari, C, Gambetti, C, Sfrappini, M, Semeraro, L, Striuli, R, Pelliccioni, G, Marinelli, D, Fabi, K, Rossi, T, Pesallaccia, M, Sabbatini, D, Gobbi, B, Cerqua, R, Tagliani, G, Schlauser, E, Caser, L, Caramello, E, Sandigliano, F, Rosso, G, Ferrari, A, Bendini, C, Luisa, D, Casella, M, Prampolini, R, Scevola, M, Vitale, E, Roberto, B, Carlo, F, Sergio, F, Alberto, S, Daniela, Z, Giulia, B, Serena, G, Michele, B, Maugeri, D, Sorace, R, Anzaldi, M, De Gesu, R, Morrone, G, Davolio, F, Fabbo, A, Palmieri, M, Zoli, M, Forti, P, Pirazzoli, L, Fabbri, E, Terenzi, L, Bergolari, F, Wenter, C, Ruffini, I, Insam, M, Abraham, E, Kirchlechner, C, Cucinotta, D, Antonino, L, Basile, G, Grazia, A, Parise, P, Boccali, A, Amici, S, Gambacorta, M, Lasagni, A, Lovati, R, Giovinazzo, F, Kimak, E, Zappa, P, Medici, F, Lo Castro, M, Mauro, F, De Luca, A, Sancesario, G, Martorana, A, Scaricamazza, B, Toniolo, S, Di Lorenzo, F, Liguori, C, Lasco, A, Vita, N, Giomi, M, Forte, F, Padovani, A, Rozzini, L, Ceraso, A, Salvatore, C, Cottino, M, Vitali, S, Marelli, E, Tripi, G, Miceli, S, Urso, G, Grioni, G, Vezzadini, G, Misaggi, G, Forlani, C, Avanzi, S, Serena, S, Claudia, C, Marilena, V, Alberto, L, Diego, G, Alessandro, G, Iemolo, F, Sanzaro, E, D'Asta, G, Proietto, M, Carnemolla, A, Razza, G, Spadaro, D, Bertolotti, M, Mussi, C, Neviani, F, Roberto, C, Valentina, G, Linda, M, Francesca, V, Tarozzi, A, Balestri, F, Mannarino, G, Bigolari, M, Natale, A, Grassi, S, Bottaro, C, Stefanelli, S, Bovone, U, Tortorolo, U, Quadri, R, Leone, G, Ponzetto, M, Frasson, P, Annoni, G, Confalonieri, R, Corsi, M, Moretti, D, Teruzzi, F, Umidi, S, Mazzola, P, Perego, S, Persico, I, Olivieri, G, Bonfanti, A, Hajnalka, S, Galeazzi, M, Massariello, F, Anzuini, A, Caffarra, P, Barocco, F, Spallazzi, M, Paolo, C, Simonetta, M, Chioatto, P, Bortolamei, S, Soattin, L, Ruotolo, G, Beneamino, B, Giuseppe, B, Bertazzoli, M, Rota, E, Adobati, A, Scarpa, A, Granziera, S, Zuccher, P, Fabbro, A, Zara, D, Lo Nigro, A, Franchetti, L, Toniolo, M, Marcuzzo, C, Rollone, M, Guerriero, F, Sgarlata, C, Masse, A, Zatti, G, Piatti, M, Graci, J, Benati, G, Boschi, F, Biondi, M, Fiumi, N, Erika, T, Locatelli, S, Mauri, S, Beretta, M, Margheritis, L, Desideri, G, Liberatore, E, Carucci, A, Bonino, P, Caput, M, Antonietti, M, Polistena, G, De la Pierre, F, Mari, M, Massignani, P, Tombesi, F, Selvaggio, F, Verbo, B, Bodoni, P, Marchionni, N, Sabatini, T, Mussio, E, Magni, E, Bianchetti, A, Crucitti, A, Titoldini, G, Cossu, B, Fascendini, S, Licini, C, Tomasoni, A, Calderazzo, M, Daniela, T, Valentina, L, Melotti, R, Lilli, A, Buda, S, Adversi, M, Noro, G, Turco, R, Ubezio, M, Mantovani, A, Viola, M, Serrati, C, Pretta, S, Infante, M, Gentile, S, D'Ambrosio, V, Mazzanti, P, Brambilla, C, Sportelli, S, Platto, C, Faraci, B, Quattrocchi, D, Pernigotti, L, Pisu, C, Sicuro, F, Zagnoni, P, Ghiglia, S, Mosca, M, Corazzin, I, Deola, M, Biagini, C, Bencini, F, Cantini, C, Tonon, E, Pierinelli, S, Onofrj, M, Thomas, A, Filomena, B, Bonanni, L, Gabriella, C, Comi, G, Magnani, G, Santangelo, R, Mazzeo, S, Francesca, C, Giordano, C, Roberto, S, Barbieri, C, Giroldi, L, Bandini, F, Masina, M, Malservisi, S, Cicognani, A, Ricca, L, Piccininni, M, Tassinari, T, Brogi, D, Sugo, A, Alessandra, F, Sonia, M, Valerio, V, Andrea, U, Enrico, C, Vera, R, Assunta, S, Gianmaria, Z, Mauro, P, Barone, A, Razzano, M, Giuseppe, I, Angela, B, Francesco, S, Valeria, D, Federico, G, Lucia, P, Antonella, V, Elisabetta, D, Cristina, R, Nadia, C, Maria, S, Luciano, A, Chiara, C, Bini, P, Pignata, M, Enrico, B, Maria, V, Giovanni, C, Giorgio, C, Piera, R, Alberto, Z, Ceccon, A, Magrin, L, Marin, S, Barbara, S, Matteo, M, Caterina, P, Carla, R, Federica, G, Clara, T, Melania, C, Giampaolo, B, Stefano, G, Valeria, G, Lucia, M, Giovambattista, D, Ester, L, Cecilia, C, Maurizio, T, Nadia, B, Grillo, A, Arenare, F, Tonino, M, David, K, Giorgio, V, Ubaldo, B, Vincenzo, S, Stefano, M, Marino, F, Busonera Flavio, M, Paolo, A, Monica, M, Francesco, B, Roberto, F, Paolo, B, Durantemangoni, E, Testoni, M, Fabio, D, Loredana, S, Valeria, S, Fabiano, M, Annabella, D, Salvatore, D, Greco, A, Grazia, D, Daniele, S, Gianluca, R, Renzo, G, Sergio, M, Morena, B, Vitali, M, Marina, P, Paolo, D, Cristina, S, Orlandini, F, La Regina, M, Desiree, A, Mario, B, Paola, P, Padulo, F, Cristina, M, Dario, R, Giancarla, M, Guido, R, Elena, M, Marileda, N, Igor, B, Nicole, B, Elena, R, Paolillo, C, Riccardi, A, Claudia, B, Barbara, R, Silvia, V, Oliver, B, Mauro, C, Eleonora, M, Giuseppe, P, Rosaria, T, Maria, C, Davide, D, Stefania, C, Massimo, P, Luca, S, Martina, D, Paola, V, Lia, S, Sandro, C, Valentina, D, Erminia, B, Paola, C, Romina, R, Minisola, S, Luciano, C, Pasquale, A, Ilaria, L, Guglielmo, S, Marco, E, Sara, R, Paola, A, Claudio, A, Francesco, R, Alessandro, C, Simona, M, Lara, F, Paola, R, Simonetta, C, Antonella, C, Generoso, U, Fernando, G, Giuliano, C, Emanuela, S, Mariolina, S, Alessandro, D, Giulia, L, Famularo, S, Sandini, M, Pinotti, E, Gianotti, L, Antonella, B, Giulia, P, Sante, G, Rossi, A, Rubele, S, Sant, S, Marco, V, Danila, C, Fabio, R, Bandirali, M, Nicoletta, C, Laura, B, Paolo, T, Luciano, T, Leonello, A, Margherita, S, Pierluigi, D, Laura, R, Fabiana, T, Giovanna, C, Antonino, A, Felice, C, Danilo, F, Giovanna, D, Francesco, L, Salini, S, Giorgetta, C, Giovanni, G, Gerardo, B, Silvio, R, Letizia, S, Davide, B, Rosaria, R, Maria, D, Raffaele, P, Palmieri, V, Palasciano, G, Belfiore, A, Portincasa, P, Carlo, S, Alessia, D, Valiani, V, Carolina, B, Tiziana, C, Paola, T, Ugo, P, Giacomo, P, Castellano, M, Anna, G, Elisa, C, Federica, C, Antonietta, C, Luigi, M, Fabio, L, Salvatore, B, Gelosa, G, Viviana, A, Piras, V, Andrea, C, Alessandra, B, Coen, D, Magliola, R, Milanesio, D, Muzzulini, C, Paolo, F, Marinella, T, Sofia, C, Marta, B, Siano, P, Capo, G, Napoletano, R, Cecilia, P, Mancini, C, Del Buono, C, De Bartolomeo, G, Addolorata, M, Carmen, C, Moschettini, G, Franco, M, Daniela, R, D'Amico, G, Mirella, P, Endrizzi, C, Trotta, L, Ciarambino, T, Orazio, Z, Emanuela, T, Marta, S, Thomas, F, Giacomo, T, Ignazio, D, Andrea, B, Giuseppe, O, Emanuela, F, Serena, A, Elena, D, Serena, B, Erika, N, Elena, S, Manuela, P, Francesca, A, Angelo, T, Di Santo SG, Rizzo, Maria Rosaria, Paolisso, Giuseppe, and Italian Study Group on Delirium, (ISGoD).
- Subjects
Rehabilitation hospital ,medicine.medical_specialty ,Urinary system ,Socio-culturale ,dementia ,elderly ,Motor subtypes of delirium ,Aged ,Cross-Sectional Studies ,Humans ,Inpatients ,Italy ,Delirium ,Dementia ,03 medical and health sciences ,0302 clinical medicine ,Internal medicine ,mental disorders ,medicine ,Motor subtypes of delirium, dementia, elderly ,dementia, elderly, Motor subtypes of delirium ,030212 general & internal medicine ,LS4_4 ,Medical prescription ,General Nursing ,Psychomotor learning ,business.industry ,Health Policy ,Medical record ,Memantine ,General Medicine ,medicine.disease ,Settore MED/26 - NEUROLOGIA ,Geriatrics and Gerontology ,medicine.symptom ,business ,030217 neurology & neurosurgery ,medicine.drug - Abstract
Objectives Few studies have analyzed factors associated with delirium subtypes. In this study, we investigate factors associated with subtypes of delirium only in patients with dementia to provide insights on the possible prevention and treatments. Design This is a cross-sectional study nested in the "Delirium Day" study, a nationwide Italian point-prevalence study. Setting and participants Older patients admitted to 205 acute and 92 rehabilitation hospital wards. Measures Delirium was evaluated with the 4-AT and the motor subtypes with the Delirium Motor Subtype Scale. Dementia was defined by the presence of a documented diagnosis in the medical records and/or prescription of acetylcholinesterase inhibitors or memantine prior to admission. Results Of the 1057 patients with dementia, 35% had delirium, with 25.6% hyperactive, 33.1% hypoactive, 34.5% mixed, and 6.7% nonmotor subtype. There were higher odds of having venous catheters in the hypoactive (OR 1.82, 95% CI 1.18-2.81) and mixed type of delirium (OR 2.23, CI 1.43-3.46), whereas higher odds of urinary catheters in the hypoactive (OR 2.91, CI 1.92-4.39), hyperactive (OR 1.99, CI 1.23-3.21), and mixed types of delirium (OR 2.05, CI 1.36-3.07). We found higher odds of antipsychotics both in the hyperactive (OR 2.87, CI 1.81-4.54) and mixed subtype (OR 1.84, CI 1.24-2.75), whereas higher odds of antibiotics was present only in the mixed subtype (OR 1.91, CI 1.26-2.87). Conclusions and implications In patients with dementia, the mixed delirium subtype is the most prevalent followed by the hypoactive, hyperactive, and nonmotor subtype. Motor subtypes of delirium may be triggered by clinical factors, including the use of venous and urinary catheters, and the use of antipsychotics. Future studies are necessary to provide further insights on the possible pathophysiology of delirium in patients with dementia and to address the optimization of the management of potential risk factors.
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- 2020
41. One-year follow-up of mud-bath therapy in patients with bilateral knee osteoarthritis: a randomized, single-blind controlled trial
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Fioravanti, A., Bacaro, G., Giannitti, C., Tenti, S., Cheleschi, S., Gui\delli, G. M., Pascarelli, N. A., and Galeazzi, M.
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- 2015
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42. The scar: the wind in the perfect storm—insights into the mysterious living tissue originating ventricular arrhythmias
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Pandozi, C., primary, Mariani, Marco Valerio, additional, Chimenti, C., additional, Maestrini, V., additional, Filomena, D., additional, Magnocavallo, M., additional, Straito, M., additional, Piro, A., additional, Russo, M., additional, Galeazzi, M., additional, Ficili, S., additional, Colivicchi, F., additional, Severino, P., additional, Mancone, M., additional, Fedele, F., additional, and Lavalle, C., additional
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- 2022
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43. Thermal Properties of Holmium-Implanted Gold Films
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Prasai, K., Alves, E., Bagliani, D., Yanardag, S. Basak, Biasotti, M., Galeazzi, M., Gatti, F., Gomes, M. Ribeiro, Rocha, J., and Uprety, Y.
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- 2014
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44. Probing the mass and anisotropy of the Milky Way gaseous halo: sight-lines toward Mrk 421 and PKS 2155-304
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Gupta, A., Mathur, S., Galeazzi, M., and Krongold, Y.
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- 2014
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45. Immunometabolic biomarkers of inflammation in Behçetʼs disease: relationship with epidemiological profile, disease activity and therapeutic regimens
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Cantarini, L., Pucino, V., Vitale, A., Talarico, R., Lucherini, O. M., Magnotti, F., De Rosa, V., Galgani, M., Alviggi, C., Marone, G., Galeazzi, M., and Matarese, G.
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- 2016
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46. High Resolution Spectroscopy of the X-Ray Emission of GRBs by IMXS-BOSS on the ISS
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Piro, L., Colasanti, L., Costa, E., Gandolfi, G., Soffitta, P., Gatti, F., Razeti, M., Pergolesi, D., Vaccarone, R., Testera, G., Pallavicini, M., Ferrari, A., Trussoni, E., Orio, M., Cammon, D. Mc, Sanders, T., Galeazzi, M., Szymkowiak, A., Porter, S., Costa, Enrico, editor, Frontera, Filippo, editor, and Hjorth, Jens, editor
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- 2001
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47. Ultrasonographic and functional changes of the ulnar nerve at Guyon’s canal after carpal tunnel release
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Ginanneschi, F., Filippou, G., Reale, F., Scarselli, C., Galeazzi, M., and Rossi, A.
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- 2010
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48. PE.Di-016 - Caractéristiques à l’inclusion et maintien d’abatacept chez les patients français présentant une Polyarthrite Rhumatoïde comparés aux patients des autres pays : analyse intermédiaire à 12 mois de l’étude internationale prospective en vie réelle ACTION
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Mariette, X., Alten, R., Nüßlein, H.G., Galeazzi, M., Lorenz, H.M., Cantagrel, A., Chartier, M., Chelbani, L., Heitzmann, J., Rauch, C., and Le Bars, M.
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- 2016
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49. PE.Di-013 - Les facteurs prédictifs du maintien d’abatacept IV dépendent-ils de la ligne de traitement de la polyarthrite rhumatoïde ? Analyse intermédiaire à 12 mois de l’étude observationnelle et prospective ACTION
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Mariette, X., Cantagrel, A., Alten, R., Nüßlein, H.G., Galeazzi, M., Lorenz, H.M., Chartier, M., Elbez, Y., Rauch, C., and Le Bars, M.
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- 2016
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50. PE.Di-012 - Le passage d’abatacept intraveineux (IV) à sous-cutané (SC) est-il durable dans la vie réelle ? Analyse à 1 an de l’étude internationale prospective ACTION
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Mariette, X., Cantagrel, A., Alten, R., Nüßlein, H.G., Galeazzi, M., Lorenz, H.M., Chartier, M., Elbez, Y., Rauch, C., and Le Bars, M.
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- 2016
- Full Text
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