Time domain astronomy with the THESEUS satellite

被引:0
|
作者
S. Mereghetti
S. Balman
M. Caballero-Garcia
M. Del Santo
V. Doroshenko
M. H. Erkut
L. Hanlon
P. Hoeflich
A. Markowitz
J. P. Osborne
E. Pian
L. Rivera Sandoval
N. Webb
L. Amati
E. Ambrosi
A. P. Beardmore
A. Blain
E. Bozzo
L. Burderi
S. Campana
P. Casella
A. D’Aí
F. D’Ammando
F. De Colle
M. Della Valle
D. De Martino
T. Di Salvo
M. Doyle
P. Esposito
F. Frontera
P. Gandhi
G. Ghisellini
D. Gotz
V. Grinberg
C. Guidorzi
R. Hudec
R. Iaria
L. Izzo
G. K. Jaisawal
P.G. Jonker
A. K. H. Kong
M. Krumpe
P. Kumar
A. Manousakis
A. Marino
A. Martin-Carrillo
R. Mignani
G. Miniutti
C. G. Mundell
K. Mukai
机构
[1] INAF,Faculty of Science, Department of Astronomy and Space Sciences
[2] IASF-Milano,Feza Gursey Center for Physics and Mathematics
[3] Istanbul University,Centre for Space Research & School of Physics
[4] Instituto de Astrofísica de Andalucía (IAA-CSIC),Dept. of Physics
[5] INAF,Center for Astrophysics and Space Sciences
[6] IASF-Palermo,School of Physics & Astronomy
[7] Institut fuer Astronomie und Astrophysik Tuebingen,Department of Astronomy
[8] Space Research Institute of the Russian Academy of Sciences,Dipartimento di Fisica
[9] Bogazici University,Instituto de Ciencias Nucleares
[10] University College Dublin,School of Physics & Astronomy
[11] Florida State University,AIM
[12] Centrum Astronomiczne im. Mikołaja Kopernika,CEA/DRF/Irfu/Département d’Astrophysique, CNRS
[13] Polskiej Akademii Nauk,Faculty of Electrical Engineering
[14] University of California,Astronomical Institute
[15] San Diego,DARK, Niels Bohr Institute
[16] University of Leicester,National Space Institute
[17] INAF,Department of Astrophysics/IMAPP
[18] Astrophysics and Space Science Observatory,Institute of Astronomy
[19] University of Alberta,Department of Applied Physics & Astronomy, College of Sciences & Sharjah Academy for Astronomy, Space Sciences, and Technology
[20] Institut de Recherche en Astrophysique et Planétologie,Department of Physics
[21] University of Geneva,Department of Physics
[22] Università degli Studi di Cagliari,Department of Mathematics and Physics Ennio De Giorgi
[23] INAF,Department of Astronomy
[24] Osservatorio Astronomico di Brera,Núcleo de Astronomía, Facultad de Ingeniería y Ciencias
[25] INAF,Department of Physics and Astronomy
[26] Osservatorio Astronomico di Roma,Physics Department
[27] INAF,Anton Pannekoek Institute for Astronomy
[28] Istituto di Radioastronomia,Mullard Space Science Laboratory
[29] Universidad Nacional Autonoma de Mexico,Department of Physics and Astronomy
[30] INAF,undefined
[31] Capodimonte Observatory,undefined
[32] Università di Palermo,undefined
[33] Scuola Universitaria Superiore IUSS Pavia,undefined
[34] University of Ferrara,undefined
[35] University of Southampton,undefined
[36] Université Paris-Saclay,undefined
[37] Université de Paris,undefined
[38] Orme des Merisiers,undefined
[39] Czech Technical University in Prague,undefined
[40] Czech Academy of Sciences,undefined
[41] Kazan Federal University,undefined
[42] University of Copenhagen,undefined
[43] Technical University of Denmark,undefined
[44] SRON,undefined
[45] Netherlands Institute for Space Research,undefined
[46] Radboud University,undefined
[47] National Tsing Hua University,undefined
[48] Leibniz-Institut für Astrophysik Potsdam,undefined
[49] University of Texas,undefined
[50] University of Sharjah,undefined
来源
Experimental Astronomy | 2021年 / 52卷
关键词
X-ray sources; Variability; X-rays surveys;
D O I
暂无
中图分类号
学科分类号
摘要
THESEUS is a medium size space mission of the European Space Agency, currently under evaluation for a possible launch in 2032. Its main objectives are to investigate the early Universe through the observation of gamma-ray bursts and to study the gravitational waves electromagnetic counterparts and neutrino events. On the other hand, its instruments, which include a wide field of view X-ray (0.3-5 keV) telescope based on lobster-eye focussing optics and a gamma-ray spectrometer with imaging capabilities in the 2-150 keV range, are also ideal for carrying out unprecedented studies in time domain astrophysics. In addition, the presence onboard of a 70 cm near infrared telescope will allow simultaneous multiwavelegth studies. Here we present the THESEUS capabilities for studying the time variability of different classes of sources in parallel to, and without affecting, the gamma-ray bursts hunt.
引用
收藏
页码:309 / 406
页数:97
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