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1. Collaborative experience between scientific software projects using Agile Scrum development

Author

Baxter, Amanda L., Benzvi, Segev Y., Walter, Bonivento, Adam, Brazier, Michael, Clark, Alexis, Coleiro, David, Collom, Marta, Colomer???molla, Bryce, Cousins, Aliwen Delgado Orellana, Damien, Dornic, Vladislav, Ekimtcov, Shereen, Elsayed, Andrea Gallo Rosso, Patrick, Godwin, Spencer, Griswold, Alec, Habig, Remington, Hill, Shunsaku, Horiuchi, Andrew Howell, D., Johnson, Margaret W. G., Mario, Juri??, Kneller, James P., Abigail, Kopec, Claudio, Kopper, Vladimir, Kulikovskiy, Mathieu, Lamoureux, Lang, Rafael F., Shengchao, Li, Massimiliano, Lincetto, Lindy, Lindstrom, Linvill, Mark W., Curtis, Mccully, Jost, Migenda, Danny, Milisavljevic, Spencer, Nelson, Rita, Novoseltseva, Erin, O'Sullivan, Donald, Petravick, Pointon, Barry W., Nirmal, Raj, Andrew, Renshaw, Janet, Rumleskie, Tom, Sonley, Ron, Tapia, Tseng, Jeffrey C. L., Tunnell, Christopher D., Godefroy, Vannoye, Vigorito, Carlo F., Virtue, Clarence J., Christopher, Weaver, Weil, Kathryn E., Lindley, Winslow, Rich, Wolski, Xun??? Jie Xu, Yiyang, Xu, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), SCiMMA, and SNEWS 2.0

Subjects
FOS: Computer and information sciences, Agile, Programvaruteknik, cyberinfrastructure, Software Engineering, FOS: Physical sciences, multimessenger astrophysics, scientific computing, software development, Software Engineering (cs.SE), Computer Science - Software Engineering, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Software
Abstract

Developing sustainable software for the scientific community requires expertise in software engineering and domain science. This can be challenging due to the unique needs of scientific software, the insufficient resources for software engineering practices in the scientific community, and the complexity of developing for evolving scientific contexts. While open-source software can partially address these concerns, it can introduce complicating dependencies and delay development. These issues can be reduced if scientists and software developers collaborate. We present a case study wherein scientists from the SuperNova Early Warning System collaborated with software developers from the Scalable Cyberinfrastructure for Multi-Messenger Astrophysics project. The collaboration addressed the difficulties of open-source software development, but presented additional risks to each team. For the scientists, there was a concern of relying on external systems and lacking control in the development process. For the developers, there was a risk in supporting a user-group while maintaining core development. These issues were mitigated by creating a second Agile Scrum framework in parallel with the developers' ongoing Agile Scrum process. This Agile collaboration promoted communication, ensured that the scientists had an active role in development, and allowed the developers to evaluate and implement the scientists' software requirements. The collaboration provided benefits for each group: the scientists actuated their development by using an existing platform, and the developers utilized the scientists' use-case to improve their systems. This case study suggests that scientists and software developers can avoid scientific computing issues by collaborating and that Agile Scrum methods can address emergent concerns., Revisions: in response to peer-review recommendations, most sections have been substantially expanded and reworked, five new figures have been added, and the title has been changed. Results unchanged

Published
2022

2. Overview of the DESI Legacy Imaging Surveys

Author

Dey, Arjun, Schlegel, David J, Lang, Dustin, Blum, Robert, Burleigh, Kaylan, Fan, Xiaohui, Findlay, Joseph R, Finkbeiner, Doug, Herrera, David, Juneau, Stéphanie, Landriau, Martin, Levi, Michael, McGreer, Ian, Meisner, Aaron, Myers, Adam D, Moustakas, John, Nugent, Peter, Patej, Anna, Schlafly, Edward F, Walker, Alistair R, Valdes, Francisco, Weaver, Benjamin A, Yèche, Christophe, Zou, Hu, Zhou, Xu, Abareshi, Behzad, Abbott, TMC, Abolfathi, Bela, Aguilera, C, Alam, Shadab, Allen, Lori, Alvarez, A, Annis, James, Ansarinejad, Behzad, Aubert, Marie, Beechert, Jacqueline, Bell, Eric F, BenZvi, Segev Y, Beutler, Florian, Bielby, Richard M, Bolton, Adam S, Briceño, César, Buckley-Geer, Elizabeth J, Butler, Karen, Calamida, Annalisa, Carlberg, Raymond G, Carter, Paul, Casas, Ricard, Castander, Francisco J, Choi, Yumi, Comparat, Johan, Cukanovaite, Elena, Delubac, Timothée, DeVries, Kaitlin, Dey, Sharmila, Dhungana, Govinda, Dickinson, Mark, Ding, Zhejie, Donaldson, John B, Duan, Yutong, Duckworth, Christopher J, Eftekharzadeh, Sarah, Eisenstein, Daniel J, Etourneau, Thomas, Fagrelius, Parker A, Farihi, Jay, Fitzpatrick, Mike, Font-Ribera, Andreu, Fulmer, Leah, Gänsicke, Boris T, Gaztanaga, Enrique, George, Koshy, Gerdes, David W, Gontcho, Satya Gontcho A, Gorgoni, Claudio, Green, Gregory, Guy, Julien, Harmer, Diane, Hernandez, M, Honscheid, Klaus, Huang, Lijuan, James, David J, Jannuzi, Buell T, Jiang, Linhua, Joyce, Richard, Karcher, Armin, Karkar, Sonia, Kehoe, Robert, Jean-Paul, Kneib, Kueter-Young, Andrea, Lan, Ting-Wen, Lauer, Tod R, Le Guillou, Laurent, Le Van Suu, Auguste, Lee, Jae Hyeon, Lesser, Michael, Levasseur, Laurence Perreault, Li, Ting S, Mann, Justin L, and Marshall, Robert

Subjects
surveys, Astronomy & Astrophysics, catalogs, Astronomical and Space Sciences, astro-ph.IM
Abstract

The DESI Legacy Imaging Surveys (http://legacysurvey.org/) are a combination of three public projects (the Dark Energy Camera Legacy Survey, the Beijing-Arizona Sky Survey, and the Mayall z-band Legacy Survey) that will jointly image ≈14,000 deg2 of the extragalactic sky visible from the northern hemisphere in three optical bands (g, r, and z) using telescopes at the Kitt Peak National Observatory and the Cerro Tololo Inter-American Observatory. The combined survey footprint is split into two contiguous areas by the Galactic plane. The optical imaging is conducted using a unique strategy of dynamically adjusting the exposure times and pointing selection during observing that results in a survey of nearly uniform depth. In addition to calibrated images, the project is delivering a catalog, constructed by using a probabilistic inference-based approach to estimate source shapes and brightnesses. The catalog includes photometry from the grz optical bands and from four mid-infrared bands (at 3.4, 4.6, 12, and 22 μm) observed by the Wide-field Infrared Survey Explorer satellite during its full operational lifetime. The project plans two public data releases each year. All the software used to generate the catalogs is also released with the data. This paper provides an overview of the Legacy Surveys project.

Published
2019

3. Overview of the DESI Legacy Imaging Surveys

Author

Dey, Arjun, Schlegel, David J., Lang, Dustin, Blum, Robert, Burleigh, Kaylan, Fan, Xiaohui, Findlay, Joseph R., Finkbeiner, Doug, Herrera, David, Juneau, Stephanie, Landriau, Martin, Levi, Michael, McGreer, Ian, Meisner, Aaron, Myers, Adam D., Moustakas, John, Nugent, Peter, Patej, Anna, Schlafly, Edward F., Walker, Alistair R., Valdes, Francisco, Weaver, Benjamin A., Yèche, Christophe, Zou, Hu, Zhou, Xu, Abareshi, Behzad, Abbott, T. M. C., Abolfathi, Bela, Aguilera, C., Alam, Shadab, Allen, Lori, Alvarez, A., Annis, James, Ansarinejad, Behzad, Aubert, Marie, Beechert, Jacqueline, Bell, Eric F., BenZvi, Segev Y., Beutler, Florian, Bielby, Richard M., Bolton, Adam S., Briceño, César, Buckley-Geer, Elizabeth J., Butler, Karen, Calamida, Annalisa, Carlberg, Raymond G., Carter, Paul, Casas, Ricard, Castander, Francisco J., Choi, Yumi, Comparat, Johan, Cukanovaite, Elena, Delubac, Timothee, DeVries, Kaitlin, Dey, Sharmila, Dhungana, Govinda, Dickinson, Mark, Ding, Zhejie, Donaldson, John B., Duan, Yutong, Duckworth, Christopher J., Eftekharzadeh, Sarah, Eisenstein, Daniel J., Etourneau, Thomas, Fagrelius, Parker A., Farihi, Jay, Fitzpatrick, Mike, Font-Ribera, Andreu, Fulmer, Leah, Gansicke, Boris T., Gaztanaga, Enrique, George, Koshy, Gerdes, David W., Gontcho, Satya Gontcho A., Gorgoni, Claudio, Green, Gregory, Guy, Julien, Harmer, Diane, Hernandez, M., Honscheid, Klaus, Lijuan, Huang, W., James, David, Jannuzi, Buell T., Jiang, Linhua, Joyce, Richard, Karcher, Armin, Karkar, Sonia, Kehoe, Robert, Kneib, Jean-Paul, Kueter-Young, Andrea, Lan, Ting-Wen, Lauer, Tod, Guillou, Laurent Le, Suu, Auguste Le Van, Lee, Jae Hyeon, Lesser, Michael, Levasseur, Laurence Perreault, Li, Ting S., Mann, Justin L., Marshall, Bob, Martinez-Vazquez, C. E., Martini, Paul, Bourboux, Helion du Mas des, McManus, Sean, Meier, Tobias Gabriel, Menard, Brice, Metcalfe, Nigel, Munoz-Gutierrez, Andrea, Najita, Joan, Napier, Kevin, Narayan, Gautham, Newman, Jeffrey A., Nie, Jundan, Nord, Brian, Norman, Dara J., Olsen, Knut A. G., Paat, Anthony, Palanque-Delabrouille, Nathalie, Peng, Xiyan, Poppett, Claire L., Poremba, Megan R., Prakash, Abhishek, Rabinowitz, David, Raichoor, Anand, Rezaie, Mehdi, Robertson, A. N., Roe, Natalie A., Ross, Ashley J., Ross, Nicholas P., Rudnick, Gregory, Safonova, Sasha, Saha, Abhijit, Sanchez, F. Javier, Savary, Elodie, Schweiker, Heidi, Scott, Adam, Seo, Hee-Jong, Shan, Huanyuan, Silva, David R., Slepian, Zachary, Soto, Christian, Sprayberry, David, Staten, Ryan, Stillman, Coley M., Stupak, Robert J., Summers, David L., Tie, Suk Sien, Tirado, H., Vargas-Magana, Mariana, Vivas, A. Katherina, Wechsler, Risa H., Williams, Doug, Yang, Jinyi, Yang, Qian, Yapici, Tolga, Zaritsky, Dennis, Zenteno, A., Zhang, Kai, Zhang, Tianmeng, Zhou, Rongpu, Zhou, Zhimin, Lawrence Berkeley National Laboratory [Berkeley] (LBNL), Universidad Antonio Nariño (UAN), Département d'Astrophysique (ex SAP) (DAP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, National University of Defense Technology [China], Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Departamento de FisicaTeorica e IFT-UAM/CSIC, Universidad Autónoma de Madrid (UAM), EPFL Laboratoire d’astrophysique, Ecole Polytechnique Fédérale de Lausanne (EPFL), National Optical Astronomy Observatory (NOAO), Columbia University [New York], Institut de Ciencies de l'Espai [Barcelona] (ICE-CSIC), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC), Biologie des Interactions Neurones / Glie, Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de la Santé et de la Recherche Médicale (INSERM), University of Arizona, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Astrophysique de Toulouse-Tarbes (LATT), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Sorbonne Université (SU), Department of Physics and Astronomy [Pittsburgh], University of Pittsburgh (PITT), Pennsylvania Commonwealth System of Higher Education (PCSHE)-Pennsylvania Commonwealth System of Higher Education (PCSHE), Galaxies, Etoiles, Physique, Instrumentation (GEPI), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut Lagrange de Paris, Chimie, Modélisation et Imagerie pour la Biologie [Orsay], Université Paris-Sud - Paris 11 (UP11)-Institut Curie [Paris]-Institut National de la Santé et de la Recherche Médicale (INSERM)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS), Computer Vision Center (Centre de visio per computador) (CVC), Universitat Autònoma de Barcelona (UAB), APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Ministry of Education Key Laboratory of Protein Sciences, Center for Structural Biology, Laboratoire de Tribologie et Dynamique des Systèmes (LTDS), École Centrale de Lyon (ECL), Université de Lyon-Université de Lyon-École Nationale des Travaux Publics de l'État (ENTPE)-Ecole Nationale d'Ingénieurs de Saint Etienne (ENISE)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Universidad Autonoma de Madrid (UAM), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de la Santé et de la Recherche Médicale (INSERM)-Institut National de la Santé et de la Recherche Médicale (INSERM), Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université de Lyon-Université de Lyon-École Nationale des Travaux Publics de l'État (ENTPE)-Ecole Nationale d'Ingénieurs de Saint Etienne-Centre National de la Recherche Scientifique (CNRS), National Natural Science Foundation of China, Department of Energy (US), National Energy Research Scientific Computing Center (US), National Science Foundation (US), National Optical Astronomy Observatory (US), Lawrence Berkeley National Laboratory, Harvard University, Dey, Arjun, Schlegel, David J., Lang, Dustin, Blum, Robert, Fan, Xiaohui, Finkbeiner, Douglas, Herrera, David, Juneau, Stephanie, Landriau, Martin, Levi, Michael, McGreer, Ian, Meisner, Aaron, Moustakas, John, Nugent, Peter, Schlafly, Edward F., Walker, Alistair, Valdés, Francisco, Zou, Hu, Abolfathi, Bela, Allen, Lori, Annis, James, Ansarinejad, Behzad, Bell, Eric F., BenZvi, Segev, Beutler, Florian, Calamida, Annalisa, Carlberg, Raymond G., Casas, Richard, Castander, Francisco J., Choi, Yumi, Dickinson, Mark, Duan, Yutong, Fagrelius, Parker, Farihi, Jay, Fulmer, Leah, Gaztañaga, Enrique, George, Koshy, Gerdes, David W., Green, Gregory, James, David J., Jannuz, Buell T., Jiang, Linhua, Joyce, Richard, Karkar, Sonia, Kehoe, Robert, Lan, Ting-Wen, Lauer, Tod R., Le Guillou, Laurent, Lesser, Michael, Marshall, Robert, Martini, Paul, Mas des Bourboux, Hélion du, Metcalfe, Nigel, Narayan, Gautham, Newman, Jeffrey A., Nord, Brian, Olsen, Knut, Prakash, Abhishek, Ross, Nicholas P., Rudnick, Gregory, Safonova, Sasha, Saha, Abhijit, Schweiker, Heidi, Silva, David R., Sien, Suk, Vivas, Kathy, Yang, Jinyi, Yang, Qian, Yapici, Tolga, Zaritsky, Dennis, Zhang, Kai, Zhang, Tianmeng, Zhou, Rongpu, University of St Andrews. School of Physics and Astronomy, Dey, Arjun [0000-0002-4928-4003], Schlegel, David J. [0000-0002-5042-5088], Lang, Dustin [0000-0002-1172-0754], Blum, Robert [0000-0002-8622-4237], Fan, Xiaohui [0000-0003-3310-0131], Finkbeiner, Douglas [0000-0003-2808-275X], Herrera, David [0000-0003-2092-6727], Juneau, Stephanie [0000-0002-0000-2394], Landriau, Martin [0000-0003-1838-8528], Levi, Michael [0000-0003-1887-1018], McGreer, Ian [0000-0002-3461-5228], Meisner, Aaron [0000-0002-1125-7384], Moustakas, John [0000-0002-2733-4559], Nugent, Peter [0000-0002-3389-0586], Schlafly, Edward F. [0000-0002-3569-7421], Walker, Alistair [0000-0002-7123-8943], Valdés, Francisco [0000-0001-5567-1301], Zou, Hu [0000-0002-6684-3997], Abolfathi, Bela [0000-0003-1820-8486], Allen, Lori [0000-0002-7789-5119], Annis, James [0000-0002-0609-3987], Ansarinejad, Behzad [0000-0002-6443-3396], Bell, Eric F. [0000-0002-5564-9873], BenZvi, Segev [0000-0001-5537-4710], Beutler, Florian [0000-0003-0467-5438], Calamida, Annalisa [0000-0002-0882-7702], Carlberg, Raymond G. [0000-0002-7667-0081], Casas, Richard [0000-0002-8165-5601], Castander, Francisco J. [0000-0001-7316-4573], Choi, Yumi [0000-0003-1680-1884], Dickinson, Mark [0000-0001-5414-5131], Duan, Yutong [0000-0002-2611-0895], Fagrelius, Parker [0000-0001-6974-5826], Farihi, Jay [0000-0003-1748-602X], Fulmer, Leah [0000-0001-9247-7794], Gaztañaga, Enrique [0000-0001-9632-0815], George, Koshy [0000-0002-1734-8455], Gerdes, David W. [0000-0001-6942-2736], Green, Gregory [0000-0001-5417-2260], James, David J. [0000-0001-5160-4486], Jannuz, Buell T. [0000-0002-1578-6582], Jiang, Linhua [0000-0003-4176-6486], Joyce, Richard [0000-0003-0201-5241], Karkar, Sonia [0000-0003-2832-777X], Kehoe, Robert [0000-0002-7101-697X], Lan, Ting-Wen [0000-0001-8857-7020], Lauer, Tod R. [0000-0003-3234-7247], Le Guillou, Laurent [0000-0001-7178-8868], Lesser, Michael [0000-0002-7199-0537], Marshall, Robert [0000-0002-6880-9987], Martini, Paul [0000-0002-4279-4182], Mas des Bourboux, Hélion du [0000-0001-8955-3573], Metcalfe, Nigel [0000-0001-9034-4402], Narayan, Gautham [0000-0001-6022-0484], Newman, Jeffrey A. [0000-0001-8684-2222], Nord, Brian [0000-0001-6706-8972], Olsen, Knut [0000-0002-7134-8296], Prakash, Abhishek [0000-0003-4451-4444], Ross, Nicholas P. [0000-0003-1830-6473], Rudnick, Gregory [0000-0001-5851-1856], Safonova, Sasha [0000-0002-2240-7421], Saha, Abhijit [0000-0002-6839-4881], Schweiker, Heidi [0000-0001-9580-4869], Silva, David R. [0000-0002-7678-2155], Sien, Suk [0000-0002-5249-1353], Vivas, Kathy [0000-0003-4341-6172], Yang, Jinyi [0000-0001-5287-4242], Yang, Qian [0000-0002-6893-3742], Yapici, Tolga [0000-0002-5306-4804], Zaritsky, Dennis [0000-0002-5177-727X], Zhang, Kai [0000-0002-9808-3646], Zhang, Tianmeng [0000-0002-8531-5161], Zhou, Rongpu [0000-0001-5381-4372], Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), and Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Université Fédérale Toulouse Midi-Pyrénées-Météo-France -Institut de Recherche pour le Développement (IRD)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)

Subjects
010504 meteorology & atmospheric sciences, [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], media_common.quotation_subject, halo, FOS: Physical sciences, Surveys, 01 natural sciences, milky-way tomography, Footprint, Software, surveys, Observatory, 0103 physical sciences, QB Astronomy, redshift distributions, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, dark energy survey, STFC, QB, 0105 earth and related environmental sciences, Remote sensing, media_common, business.industry, RCUK, Astronomy and Astrophysics, cosmos, 3rd-DAS, Probabilistic inference, Galactic plane, streams, Photometry (astronomy), Space and Planetary Science, Sky, Satellite, digital sky survey, galaxy, Catalogs, Astrophysics - Instrumentation and Methods for Astrophysics, business, sdss, sextractor, catalogs, Geology, astro-ph.IM
Abstract

The DESI Legacy Imaging Surveys (http://legacysurvey.org/) are a combination of three public projects (the Dark Energy Camera Legacy Survey, the Beijing-Arizona Sky Survey, and the Mayall z-band Legacy Survey) that will jointly image ≈14,000 deg2 of the extragalactic sky visible from the northern hemisphere in three optical bands (g, r, and z) using telescopes at the Kitt Peak National Observatory and the Cerro Tololo Inter-American Observatory. The combined survey footprint is split into two contiguous areas by the Galactic plane. The optical imaging is conducted using a unique strategy of dynamically adjusting the exposure times and pointing selection during observing that results in a survey of nearly uniform depth. In addition to calibrated images, the project is delivering a catalog, constructed by using a probabilistic inference-based approach to estimate source shapes and brightnesses. The catalog includes photometry from the grz optical bands and from four mid-infrared bands (at 3.4, 4.6, 12, and 22 μm) observed by the Wide-field Infrared Survey Explorer satellite during its full operational lifetime. The project plans two public data releases each year. All the software used to generate the catalogs is also released with the data. This paper provides an overview of the Legacy Surveys project., The BASS is also supported by the External Cooperation Program of Chinese Academy of Sciences (Grant # 114A11KYSB20160057), and Chinese National Natural Science Foundation (Grant # 11433005). The Legacy Surveys imaging of the DESI footprint is supported by the Director, Office of Science, Office of High Energy Physics of the U.S. Department of Energy under Contract No. DE-AC02- 05CH11231, by the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility under the same contract; and by the U.S. National Science Foundation, Division of Astronomical Sciences under Contract No. AST-0950945 to NOAO. Travel and other support for the DECaLS and MzLS projects is provided by the National Optical Astronomy Observatory, the Lawrence Berkeley National Laboratory, and the DESI Project. This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. The research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Programme (FP/2007-2013) / ERC Grant Agreement n. 320964 (WDTracer). J. Moustakas gratefully acknowledges support from the National Science Foundation grant AST1616414. A. Dey thanks the Radcliffe Institute for Advanced Study for their generous support during the year these surveys were initiated. A. Dey, D. J. Schlegel, and D. Lang thank the Aspen Center for Physics, which is supported by National Science Foundation grant PHY-1066293, for their hospitality and support during summer 2015 during which part of this work was conducted.

Published
2019

4. Dielectric Relaxation of Hydration Water in Native Collagen Fibrils

Author

Kurzweil-Segev Y., Popov I., Solomonov I., Sagit I., and Feldman Y.

Abstract

© 2017 American Chemical Society. The dielectric relaxation of hydrated collagen powders was studied over a wide temperature and frequency range. We revealed two mechanisms of dielectric relaxation in hydration water that are driven by the migration of ionic and orientation defects. At high water fractions in powders (h > 0.2), the hydration shell around the collagen triple helixes presents a spatial H-bonded network consisting of structural water bridges and cleft water channels. These two water phases provide the long-range paths for proton hopping and orientation defect migration. At low water fractions (h < 0.2) and in the hydrated collagen samples after the dehydrothermal treatment, the hydration shell presents localized individual water compartments not connected to one another. In these cases, the relaxation mechanism due to proton hopping either disappears or becomes inhibited by the orientation defect migration.

Published
2017

5. Confined water dynamics in a hydrated photosynthetic pigment-protein complex

Author

Kurzweil-Segev Y., Popov I., Eisenberg I., Yochelis S., Keren N., Paltiel Y., and Feldman Y.

Subjects
macromolecular substances
Abstract

© This journal is the Owner Societies. Water is of fundamental importance for life. It plays a critical role in all biological systems. In p hycocyanin, a pigment-protein complex, the hydration level influences its absorption spectrum. However, there is currently a gap in the understanding of how protein interfaces affect water's structure and properties. This work presents combined dielectric and calorimetric measurements of hydrated phycocyanin with different levels of hydration in a broad temperature interval. Based on the dielectric and calorimetric tests, it was shown that two types of water exist in the phycocyanin hydration shell. One is confined water localized inside the phycocyanin ring and the second is the water that is embedded in the protein structure and participates in the protein solvation. The water confined in the phycocyanin ring melts at the temperature 195 ± 3 K and plays a role in the solvation at higher temperatures. Moreover, the dynamics of all types of water was found to be effected by the presence of the ionic buffer.

Published
2017

6. IceTop: The surface component of IceCube. The IceCube Collaboration

Author

Abbasi Rasha U., Abdou Yasser, Ackermann Markus, Adams Jenni A., Aguilar Juan Antonio, Ahlers Markus, Altmann D., Andeen K. G., Auffenberg Jan, Bai X., Baker Michael A., Barwick Steven W., Baum V., Bay R., Beattie K., Beatty James J., Bechet S., Becker Tjus Julia, Becker Karl Heinz, Bell M., Benabderrahmane M. L., Benzvi Segev Y., Berdermann Jens, Berghaus Patrick, and Berley D.

Subjects
Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, High Energy Physics::Experiment
Abstract

IceTop the surface component of the IceCube Neutrino Observatory at the South Pole is an air shower array with an area of 1km2. The detector allows a detailed exploration of the mass composition of primary cosmic rays in the energy range from about 100TeV to 1EeV by exploiting the correlation between the shower energy measured in IceTop and the energy deposited by muons in the deep ice. In this paper we report on the technical design construction and installation the trigger and data acquisition systems as well as the software framework for calibration reconstruction and simulation. Finally the first experience from commissioning and operating the detector and the performance as an air shower detector will be discussed.

Published
2013

7. The variety of states of adsorbed water in heterogeneous materials and their dielectric response

Author

Feldman Y., Puzenko A., Ishai P., Greenbaum A., Segev Y., Vasilyeva M., and Gusev Y.

Subjects
Porous Glasses, Adsorbed Water, Cole-Cole Spectral Function, Anomalous Diffusion, Dielectric Relaxation
Abstract

Whenever water interacts with another dipolar or charged entity, there exists a broadening of its dielectric relaxation peak. Often this broadening can be described by the phenomenological Cole-Cole (CC) spectral function. A new approach has been recently presented (A. Puzenko, P. Ben Ishai, and Y. Feldman, Phys. Rev. Letters 105, 037601-4 (2010)), which is based on the fractal nature of the time set of the interaction of the relaxing water dipoles with their encompassing matrix. It demonstrates a fundamental connection between the relaxation time, τ, the broadening parameter, α, and the Kirkwood-Froehlich correlation function B. The parameters B, τ and α were chosen as the coordinates of the new 3D space, wherein the evolution of the relaxation process, as a result of the variation of external macroscopic parameters (temperature, pressure etc.), will depict a trajectory. This trajectory is a result of the connection between the kinetic and the structural properties of water in the complex system. © 2013 American Institute of Physics.

Published
2013

9. Mott insulator phases and first-order melting in BSCCO crystals with periodic surface holes

Author

Goldberg, S., Segev, Y., Myasoedov, Y., Gutman, I., Avraham, N., Rappaport, M., Zeldov, E., Tamegai, T., Hicks, C. W., and Moler, K. A.

Subjects
Superconductivity (cond-mat.supr-con), Condensed Matter::Superconductivity, Condensed Matter - Superconductivity, FOS: Physical sciences
Abstract

We measured the effects of periodic surface holes, created using a focused ion beam, on the phase diagram of the vortex matter in high-T_c Bi_2Sr_2CaCu_2O_{8+\delta} crystals. Differential magneto-optical measurements show that the irreversibility line is shifted to higher fields and temperatures, with respect to the pristine melting line. The irreversibility line displays weak field dependence between integer matching fields indicating multiple-flux-quanta pinning at holes. We find reduced equilibrium compressibility of the vortex matter at integer matching fields, which is strong evidence for the existence of thermodynamic Mott insulator phases. Shaking with a transverse ac field surprisingly reveals first-order melting that is not shifted with respect to the pristine melting line and that seems to occur within the Mott insulator regions. This melting is understood to be the first-order transition in the bulk of the crystal beneath the surface holes. The transition is visible at the surface, despite the reduced vortex compressibility in the top layer., Comment: 11 pages, 8 figures. To appear in Physical Review B

Published
2009

10. Special Moufang Sets, Their Root Groups And Their Mu-Maps

Author

De Medts, Tom, Segev, Y., and Tent, K.

Subjects
Mathematics::Group Theory
Abstract

We prove Timmesfeld's conjecture that special abstract rank one groups are quasisimple. We show that in a special Moufang set the root groups are characterized on the one hand by being regular and normal in the point stabilizer, and on the other hand a normal transitive nilpotent subgroup of the point stabilizer is a root group. We prove that if a root group of a special Moufang set contains an involution, then it is of exponent $2$. We also show that the root groups are abelian if and only if the so-called $\mu$-maps are involutions.

Published
2008
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13. Erratum: IceCube sensitivity for low-energy neutrinos from nearby supernovae(Astronomy and Astrophysics (2011) 535 : A109 (DOI: 10.1051/0004-6361/201117810))

Author

Abbasi Rasha U., Abdou Yasser, Abu-Zayyad Tareq, Ackermann Markus, Adams Jenni A., Aguilar Juan Antonio, Ahlers Markus, Allen Malcolm M., Altmann D., Andeen K. G., Auffenberg Jan, Bai X., Baker Michael A., Barwick Steven W., Baum V., Bay Ryan, Bazo Alba J. L., Beattie K., Beatty James J., Bechet S., Becker Julia K., Becker K. H., Benabderrahmane M. L., Benzvi Segev Y., and Berdermann Jens

Published
2014

15. Morphometric study of the midsagittal MR imaging plane in cases of hydrocephalus and atrophy and in normal brains

Author

Segev Y, Ur Metser, Beni-Adani L, Elran C, Ii, Reider-Groswasser, and Constantini S

Subjects
Adult, Aged, 80 and over, Adolescent, Child, Preschool, Humans, Brain, Infant, Atrophy, Middle Aged, Child, Magnetic Resonance Imaging, Aged, Hydrocephalus
Abstract

BACKGROUND AND PURPOSE: Midsagittal morphologic changes often aid in the diagnosis of hydrocephalus. Stretching and upward displacement of the corpus callosum, widening of third ventricular recesses, and decreased mammillopontine distance have been described as indicating the possibility of hydrocephalus. Quantitative studies are scarce. We performed retrospective, quantitative analysis to verify and quantify changes in midline morphology that might differentiate hydrocephalus and ventriculomegaly due to atrophy. METHODS: Sagittal MR imaging studies of 22 patients with hydrocephalus and 32 patients with atrophy were analyzed, as were 42 studies with normal findings. The studied parameters included mammillopontine and mammillocommissural distances, callosal height at two points, and the distances between the lines passing through the chiasm (chiasmal line) and the edge of the callosal splenium. Various angles between the chiasmal line and surrounding structures were measured. Similar measurements were done with the line passing through the third ventricular floor segment anterior to the mammillary bodies (third ventricular line). RESULTS: In hydrocephalus, mammillopontine distance decreased, mammillocommissural distance increased, the third ventricular floor segment was concave in most cases, and the chiasmal line rotated clockwise. These changes were not seen in atrophy. Callosal height was increased in hydrocephalus significantly more than in atrophy. CONCLUSION: Specific changes of the midsagittal plane in hydrocephalus, some of which have not been described previously, can be observed and quantified, which might aid in differentiating this condition from atrophy.

16. Clear cell carcinoma of the endometrium

Author

Giorgio Bogani, Isabelle Ray-Coquard, Nicole Concin, Natalie Y.L. Ngoi, Philippe Morice, Takayuki Enomoto, Kazuhiro Takehara, Hannelore Denys, Domenica Lorusso, Robert Coleman, Michelle M. Vaughan, Masashi Takano, Diane Provencher, Satoru Sagae, Pauline Wimberger, Robert Póka, Yakir Segev, Se Ik Kim, Jae-Weon Kim, Francisco J. Candido dos Reis, Andrea Mariani, Mario M. Leitao, Viky Makker, Nadeem Abu Rustum, Ignace Vergote, Gian Franco Zannoni, David S.P. Tan, Mary McCormack, Marta Bini, Salvatore Lopez, Francesco Raspagliesi, Pierluigi Benedetti Panici, Violante di Donato, Ludovico Muzii, Nicoletta Colombo, Giovanni Scambia, Sandro Pignata, Bradley J. Monk, Bogani, G, Ray-Coquard, I, Concin, N, Ngoi, N, Morice, P, Enomoto, T, Takehara, K, Denys, H, Lorusso, D, Coleman, R, Vaughan, M, Takano, M, Provencher, D, Sagae, S, Wimberger, P, Poka, R, Segev, Y, Kim, S, Kim, J, Candido dos Reis, F, Mariani, A, Leitao, M, Makker, V, Rustum, N, Vergote, I, Zannoni, G, Tan, D, Mccormack, M, Bini, M, Lopez, S, Raspagliesi, F, Panici, P, di Donato, V, Muzii, L, Colombo, N, Scambia, G, Pignata, S, and Monk, B

Subjects
Clear cell endometrial cancer, Immunotherapy, Target therapy, Uterine cancer, Obstetrics and Gynecology, Prognosis, Endometrial Neoplasms, Endometrium, Settore MED/40 - GINECOLOGIA E OSTETRICIA, Oncology, Uterine Neoplasms, Humans, Female, Tumor Suppressor Protein p53, Adenocarcinoma, Clear Cell
Abstract

Clear cell endometrial carcinoma represents an uncommon and poorly understood entity. Data from molecular/genomic profiling highlighted the importance of various signatures in assessing the prognosis of endometrial cancer according to four classes of risk (POLE mutated, MMRd, NSMP, and p53 abnormal). Unfortunately, data specific to clear cell histological subtype endometrial cancer are lacking. More recently, data has emerged to suggest that most of the patients (more than 80%) with clear cell endometrial carcinoma are characterized by p53 abnormality or NSMP type. This classification has important therapeutic implications. Although it is an uncommon entity, clear cell endometrial cancer patients with POLE mutation seem characterized by a good prognosis. Chemotherapy is effective in patients with NSMP (especially in stage III and IV) and patients with p53 abnormal disease (all stages). While, preliminary data suggested that patients with MMRd are less likely to benefit from chemotherapy. The latter group appears to benefit much more from immune checkpoint inhibitors: recent data from clinical trials on pembrolizumab plus lenvatinib and nivolumab plus cabozantinib supported that immunotherapy plus tyrosine kinase inhibitors (TKI) would be the most appropriate treatment for recurrent non-endometrioid endometrial cancer (including clear cell carcinoma) after the failure of platinum-based chemotherapy. Moreover, ongoing clinical trials testing the anti-tumor activity of innovative products will clarify the better strategies for advanced/recurrent clear cell endometrial carcinoma. Further prospective evidence is urgently needed to better characterize clear cell endometrial carcinoma.

Published
2022

17. Endometrial carcinosarcoma

Author

Giorgio Bogani, Isabelle Ray-Coquard, Nicole Concin, Natalie Yan Li Ngoi, Philippe Morice, Giuseppe Caruso, Takayuki Enomoto, Kazuhiro Takehara, Hannelore Denys, Domenica Lorusso, Robert Coleman, Michelle M Vaughan, Masashi Takano, Diane Michele Provencher, Satoru Sagae, Pauline Wimberger, Robert Póka, Yakir Segev, Se Ik Kim, Jae-Weon Kim, Francisco Jose Candido dos Reis, Pedro T Ramirez, Andrea Mariani, Mario Leitao, Vicky Makker, Nadeem R Abu-Rustum, Ignace Vergote, Gianfranco Zannoni, David Tan, Mary McCormack, Biagio Paolini, Marta Bini, Francesco Raspagliesi, Pierluigi Benedetti Panici, Violante Di Donato, Ludovico Muzii, Nicoletta Colombo, Sandro Pignata, Giovanni Scambia, Bradley J Monk, Bogani, G, Ray-Coquard, I, Concin, N, Ngoi, N, Morice, P, Caruso, G, Enomoto, T, Takehara, K, Denys, H, Lorusso, D, Coleman, R, Vaughan, M, Takano, M, Provencher, D, Sagae, S, Wimberger, P, Póka, R, Segev, Y, Kim, S, Kim, J, Candido Dos Reis, F, Ramirez, P, Mariani, A, Leitao, M, Makker, V, Abu-Rustum, N, Vergote, I, Zannoni, G, Tan, D, Mccormack, M, Paolini, B, Bini, M, Raspagliesi, F, Benedetti Panici, P, Di Donato, V, Muzii, L, Colombo, N, Pignata, S, Scambia, G, and Monk, B

Subjects
female, Settore MED/40 - GINECOLOGIA E OSTETRICIA, Oncology, genital neoplasms, female, genital neoplasms, Obstetrics and Gynecology, carcinosarcoma, uterine cancer
Abstract

Endometrial carcinosarcoma is a rare and aggressive high-grade endometrial carcinoma with secondary sarcomatous trans-differentiation (conversion theory). The clinical presentation and diagnostic work-up roughly align with those of the more common endometrioid counterpart, although endometrial carcinosarcoma is more frequently diagnosed at an advanced stage. Endometrial carcinosarcoma is not a single entity but encompasses different histological subtypes, depending on the type of carcinomatous and sarcomatous elements. The majority of endometrial carcinosarcomas are characterized by p53 abnormalities. The proportion ofPOLEand microsatellite instablity-high (MSI-H) is directly related to the epithelial component, being approximately 25% and 3% in endometrioid and non-endometrioid components.The management of non-metastatic disease is based on a multimodal approach with optimal surgery followed by (concomitant or sequential) chemotherapy and radiotherapy, even for early stages. Palliative chemotherapy is recommended in the metastatic or recurrent setting, with carboplatin/paclitaxel doublet being the first-line regimen. Although the introduction of immunotherapy plus/minus a tyrosine kinase inhibitor shifted the paradigm of treatment of patients with recurrent endometrial cancer, patients with endometrial carcinosarcoma were excluded from most studies evaluating single-agent immunotherapy or the combination. However, the US Food and Drug Administration (FDA) and the European Medicines Agency (EMA) approved the use of pembrolizumab and lenvatinib in endometrial cancer (all histotypes) after progression on chemotherapy and single-agent immunotherapy in MSI-H cancers. In the era of precision medicine, emerging knowledge on molecular endometrial carcinosarcoma is opening new promising therapeutic options for more personalized treatment. The present review outlines state-of-the-art knowledge and future directions for patients with endometrial carcinosarcoma.

Published
2023

18. Uterine serous carcinoma

Author

Diane Provencher, Michelle M. Vaughan, Kazuhiro Takehara, Violante Di Donato, Takayuki Enomoto, Se Ik Kim, Nicoletta Colombo, Domenica Lorusso, Nicole Concin, Natalie Ngoi, Giovanni Scambia, Francesco Raspagliesi, Isabelle Ray-Coquard, Bradley J. Monk, Róbert Póka, Ludovico Muzii, Remi A. Nout, Satoru Sagae, Andrea Mariani, Sandro Pignata, Philippe Morice, Hannelore Denys, Mario M. Leitao, Pauline Wimberger, Yakir Segev, Salvatore Lopez, Alice Indini, Francisco José Candido dos Reis, Pieluigi Benedetti Panici, Marta Bini, Giorgio Bogani, Masashi Takano, Bogani, G, Ray-Coquard, I, Concin, N, Ngoi, N, Morice, P, Enomoto, T, Takehara, K, Denys, H, Nout, R, Lorusso, D, Vaughan, M, Bini, M, Takano, M, Provencher, D, Indini, A, Sagae, S, Wimberger, P, Poka, R, Segev, Y, Kim, S, Candido dos Reis, F, Lopez, S, Mariani, A, Leitao, M, Raspagliesi, F, Panici, P, Di Donato, V, Muzii, L, Colombo, N, Scambia, G, Pignata, S, and Monk, B

Subjects
0301 basic medicine, Oncology, medicine.medical_specialty, Serous uterine cancer, medicine.medical_treatment, Gynecologic oncology, Pembrolizumab, Article, Uterine serous carcinoma, Targeted therapy, 03 medical and health sciences, chemistry.chemical_compound, 0302 clinical medicine, Endometrial cancer, SDG 3 - Good Health and Well-being, Internal medicine, Medicine, Humans, Randomized Controlled Trials as Topic, business.industry, Obstetrics and Gynecology, medicine.disease, Cystadenocarcinoma, Serous, Radiation therapy, Serous fluid, 030104 developmental biology, chemistry, Clinical Trials, Phase III as Topic, 030220 oncology & carcinogenesis, IMUNOTERAPIA, Uterine Neoplasms, Female, Immunotherapy, business, Lenvatinib
Abstract

Serous endometrial cancer represents a relative rare entity accounting for about 10% of all diagnosed endometrial cancer, but it is responsible for 40% of endometrial cancer-related deaths. Patients with serous endometrial cancer are often diagnosed at earlier disease stage, but remain at higher risk of recurrence and poorer prognosis when compared stage-for-stage with endometrioid subtype endometrial cancer. Serous endometrial cancers are characterized by marked nuclear atypia and abnormal p53 staining in immunohistochemistry. The mainstay of treatment for newly diagnosed serous endometrial cancer includes a multi-modal therapy with surgery, chemotherapy and/or radiotherapy. Unfortunately, despite these efforts, survival outcomes still remain poor. Recently, The Cancer Genome Atlas (TCGA) Research Network classified all endometrial cancer types into four categories, of which, serous endometrial cancer mostly is found within the "copy number high" group. This group is characterized by the increased cell cycle deregulation (e.g., CCNE1, MYC, PPP2R1A, PIKCA, ERBB2 and CDKN2A) and TP53 mutations (90%). To date, the combination of pembrolizumab and lenvatinib is an effective treatment modality in second-line therapy, with a response rate of 50% in advanced/recurrent serous endometrial cancer. Owing to the unfavorable outcomes of serous endometrial cancer, clinical trials are a priority. At present, ongoing studies are testing novel combinations of various targeted and immunotherapeutic agents in newly diagnosed and advanced/recurrent endometrial cancer - an important strategy for serous endometrial cancer, whereby tumors are usually p53+ and pMMR, making response to PD-1 inhibitor monotherapy unlikely. Here, the rare tumor working group (including members from the European Society of Gynecologic Oncology (ESGO), Gynecologic Cancer Intergroup (GCIG), and Japanese Gynecologic Oncology Group (JGOG)), performed a narrative review reporting on the current landscape of serous endometrial cancer and focusing on standard and emerging therapeutic options for patients affected by this difficult disease.

Published
2021

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