POEMMA: Probe Of Extreme Multi-Messenger Astrophysics
A. V. Olinto, J. H. Adams, R. Aloisio, L. A. Anchordoqui, D. R. Bergman, M. E. Bertaina, P. Bertone, M. Bustamante, M. J. Christl, S. E. Csorna, J. B. Eser, F. … 展开作者
A. V. Olinto, J. H. Adams, R. Aloisio, L. A. Anchordoqui, D. R. Bergman, M. E. Bertaina, P. Bertone, M. Bustamante, M. J. Christl, S. E. Csorna, J. B. Eser, F. Fenu, C. Guépin, E. A. Hays, S. Hunter, E. Judd, I. Jun, K. Kotera, J. F. Krizmanic, E. Kuznetsov, S. Mackovjak, L. M. Martinez-Sierra, M. Mastafa, J. N. Matthews, J. McEnery, J. W. Mitchell, A. Neronov, A. N. Otte, E. Parizot, T. C. Paul, J. S. Perkins, G. Prevot, P. Reardon, M. H. Reno, F. Sarazin, K. Shinozaki, F. Stecker, R. Streitmatter, T. Venters, L. Wiencke, R. M. Young
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8 pages, in the Proceedings of the 35th International Cosmic Ray Conference, ICRC217, Busan, Korea
The Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) mission is being designed to establish charged-particle astronomy with ultra-high energy cosmic rays (UHECRs) and to observe cosmogenic tau neutrinos (CTNs). The study of UHECRs and CTNs from space will yield orders-of-magnitude increase in statistics of observed UHECRs at the highest energies, and the observation of the cosmogenic flux of neutrinos for a range of UHECR models. These observations should solve the long-standing puzzle of the origin of the highest energy particles ever observed, providing a new window onto the most energetic environments and events in the Universe, while studying particle interactions well beyond accelerator energies. The discovery of CTNs will help solve the puzzle of the origin of UHECRs and begin a new field of Astroparticle Physics with the study of neutrino properties at ultra-high energies.
POEMMA-Balloon with Radio: A multi-messenger, multi-detector balloon payload
CSPAR, University of Alabama Huntsville（卡尔森太空物理应用研究中心，阿拉巴马大学亨茨维尔分校）；Pennsylvania State University（宾夕法尼亚州立大学）；Laboratoire APC, Université Paris Cité（巴黎西岱大学APC实验室）；RSESC, University of Alabama Huntsville（雷恩空间科学中心，阿拉巴马大学亨茨维尔分校）；Laboratori Nazionali del Gran Sasso, Istituto Nazionale di Fisica Nucleare（意大利国家核物理研究所大萨索国家实验室）；Gran Sasso Science Institute（大萨索科学研究所）；Sezione di Roma Tor Vergata, Istituto Nazionale di Fisica Nucleare（意大利国家核物理研究所罗马托尔维加塔分部）；Sezione di Napoli, Istituto Nazionale di Fisica Nucleare（意大利国家核物理研究所那不勒斯分部）；Department of Physics and Astronomy, Lehman CUNY（莱曼学院物理学与天文学系（纽约市立大学））；Institute of Experimental Physics, Slovak Academy of Sciences（斯洛伐克科学院实验物理研究所）；Department of Physics, Colorado School of Mines（科罗拉多矿业学院物理系）；Sezione di Bari, Istituto Nazionale di Fisica Nucleare（意大利国家核物理研究所巴里分部）
本文介绍了POEMMA-Balloon with Radio项目，旨在通过多信使观测研究超高能宇宙射线，利用气球载荷实现同时光学和无线电观测，为空间任务技术准备和高能宇宙射线研究提供数据支持。
Deep Learning for Multi-Messenger Astrophysics: A Gateway for Discovery in the Big Data Era
NCSA, University of Illinois at Urbana-Champaign（伊利诺伊大学厄巴纳-香槟分校国家超级计算应用中心）；Department of Astronomy, University of Illinois at Urbana-Champaign（伊利诺伊大学厄巴纳-香槟分校天文学系）；California Institute of Technology（加州理工学院）；Las Cumbres Observatory（拉斯坎布雷斯天文台）；Caltech/IPAC-NExScI（加州理工学院/红外处理与分析中心-系外行星科学研究所）；Department of Physics and Astronomy, University of Delaware（特拉华大学物理与天文学系）；Data Science Institute, University of Delaware（特拉华大学数据科学研究所）；Center for Urban Science and Progress, New York University（纽约大学城市科学与进步中心）；The Oskar Klein Centre for Cosmoparticle Physics, Stockholm University（斯德哥尔摩大学奥斯卡·克莱因宇宙粒子物理中心）；The University of Chicago（芝加哥大学）；IBM Systems（IBM系统部）
Enabling real-time multi-messenger astrophysics discoveries with deep learning
University of Illinois at Urbana-Champaign（伊利诺伊大学厄巴纳-香槟分校）；California Institute of Technology（加州理工学院）；Tecnologico de Monterrey（蒙特雷理工学院）；Las Cumbres Observatory（拉斯坎布雷斯天文台）；University of Delaware（特拉华大学）；Stockholm University（斯德哥尔摩大学）；The University of Chicago（芝加哥大学）；IBM T.J. Watson Research Center（IBM托马斯·J·沃森研究中心）；Carnegie Institute for Science（卡内基科学研究所）；West Virginia University（西弗吉尼亚大学）
LUMOS : Linear programming Utility for Multi-messenger Optical Scheduling
Astrophysics Research Institute, Liverpool John Moores University（利物浦约翰摩尔斯大学天体物理研究所）；Department of Physics, Indian Institute of Technology Bombay（印度理工学院孟买分校物理系）；School of Physics and Astronomy, University of Minnesota（明尼苏达大学物理与天文学学院）；Astrophysics Science Division, NASA Goddard Space Flight Center（NASA戈达德太空飞行中心天体物理学科学部）；Joint Space-Science Institute, University of Maryland（马里兰大学联合空间科学研究所）
Observational strategies for ultrahigh-energy neutrinos: the importance of deep sensitivity for detection and astronomy
Sorbonne Université（索邦大学）；CNRS（法国国家科学研究中心）；Institut d’Astrophysique de Paris（巴黎天体物理研究所）；Vrije Universiteit Brussels（布鲁塞尔自由大学）；The Pennsylvania State University（宾夕法尼亚州立大学）；Universite Paris Diderot（巴黎第七大学）；Laboratoire de Physique Nucleaire et de Hautes Energies（核物理与高能物理实验室）；Center for Multimessenger Astrophysics（多信使天文学中心）；Institute for Gravitation and the Cosmos（引力与宇宙研究所）
An agentic framework for gravitational-wave counterpart association in the multi-messenger era
Department of Astronomy, School of Physics（天文学系，物理系）；Kavli Institute for Astronomy and Astrophysics（天体物理研究所）；Institute for Gravitational Wave Astronomy（引力波天文研究所）；School of Information Science and Technology（信息科学与技术学院）；National Astronomical Observatories（国家天文台）
