STROBE-X: X-ray Timing and Spectroscopy on Dynamical Timescales from Microseconds to Years
Colleen A. Wilson-Hodge, Paul S. Ray, Keith Gendreau, Deepto Chakrabarty, Marco Feroci, Zaven Arzoumanian, Soren Brandt, Margarita Hernanz, C. Michelle Hui, Pet… 展开作者
Colleen A. Wilson-Hodge, Paul S. Ray, Keith Gendreau, Deepto Chakrabarty, Marco Feroci, Zaven Arzoumanian, Soren Brandt, Margarita Hernanz, C. Michelle Hui, Peter A. Jenke, Thomas Maccarone, Ron Remillard, Kent Wood, Silvia Zane
The Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays (STROBE-X) probes strong gravity for stellar mass to supermassive black holes and ultradense matter with unprecedented effective area, high time-resolution, and good spectral resolution, while providing a powerful time-domain X-ray observatory.
Mitigating the Timing Impact of Anomalous Pulse Profile Shape Variability in PSR J1713+0747 with Gaussian Component Modeling
NANOGrav Physics Frontiers Center（NANOGrav物理前沿中心）；SETI Institute（SETI研究所）；Center for Gravitation, Cosmology and Astrophysics, Department of Physics and Astronomy, University of Wisconsin-Milwaukee（威斯康星大学密尔沃基分校物理与天文学系引力、宇宙学与天体物理中心）；Department of Physics, Oregon State University（俄勒冈州立大学物理系）；Department of Physics and Astronomy, Vanderbilt University（范德堡大学物理与天文学系）；Department of Physics and Astronomy, University of British Columbia（不列颠哥伦比亚大学物理与天文学系）；Department of Physics and Astronomy, George Mason University（乔治梅森大学物理与天文学系）；National Radio Astronomy Observatory（美国国家射电天文台）；Institute of Astrophysics, FORTH（希腊基础与研究基金会天体物理研究所）
In-orbit Demonstration of X-ray Pulsar Navigation with NinjaSat
Graduate School of Advanced Science and Engineering, Hiroshima University（广岛大学先进理工学研究科）；RIKEN Pioneering Research Institute（理化学研究所先锋研究本部）；International Center for Hadron Astrophysics, Chiba University（千叶大学强子天体物理学国际中心）；Department of Physics, Tokyo Metropolitan University（东京都立大学物理学系）；Department of Physics, National Changhua University of Education（国立彰化师范大学物理学系）；Rikkyo University（立教大学）；Department of Earth and Space Science, The University of Osaka（大阪大学地球惑星科学系）
Spectroscopic performance of the electrical functional models for the eXTP SFA-T detectors
Max-Planck-Institut für extraterrestrische Physik（马克斯·普朗克地外物理学研究所）；Halbleiterlabor der Max-Planck-Gesellschaft（马克斯·普朗克学会半导体实验室）；Politecnico di Milano（米兰理工大学）
CubeSats Reach the Millisecond X-Ray Domain: Crab Pulsar Timing with SpIRIT/HERMES
University of Trento（特伦托大学）；University of Palermo（巴勒莫大学）；INAF/Osservatorio Astronomico di Trieste（意大利国家天体物理研究所的里雅斯特天文台）；School of Physics, The University of Melbourne（墨尔本大学物理学院）；Dipartimento di Fisica, Università degli Studi di Cagliari（卡利亚里大学物理系）；INAF/IASF Palermo（意大利国家天体物理研究所巴勒莫空间物理学研究所）；INAF/OAS（意大利国家天体物理研究所博洛尼亚天文台）；INFN Sezione di Bologna（意大利国家核物理研究所博洛尼组分所）
