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The THESEUS space mission concept: science case, design and expected performances
Amati, L; O'Brien, P; Gotz, D; Bozzo, E; Tenzer, C; Frontera, F; Ghirl; a, G; Labanti, C; Osborne, JP; Stratta, G; Tanvir, N; Willingale, R; Attina, P; Campana, R; Castro-Tirado, AJ; Contini, C; Fuschino, F; Gomboc, A; Hudec, R; Orleanski, P; Renotte, E; Rodic, T; Bagoly, Z; Blain, A; Callanan, P; Covino, S; Ferrara, A; Le Floch, E; Marisaldi, M; Mereghetti, S; Rosati, P; Vacchi, A; D'Avanzo, P; Giommi, P; Piranomonte, S; Piro, L; Reglero, V; Rossi, A; Santangelo, A; Salvaterra, R; Tagliaferri, G; Vergani, S; Vinciguerra, S; Briggs, M; Campolongo, E; Ciolfi, R; Connaughton, V; Cordier, B; Morelli, B; Orl; ini, M; Adami, C; Argan, A; Atteia, JL; Auricchio, N; Balazs, L; Baldazzi, G; Basa, S; Basak, R; Bellutti, P; Bernardini, MG; Bertuccio, G; Braga, J; Branchesi, M; Br; t, S; Brocato, E; Budtz-Jorgensen, C; Bulgarelli, A; Burderi, L; Camp, J; Capozziello, S; Caruana, J; Casella, P; Cenko, B; Chardonnet, P; Ciardi, B; Colafrancesco, S; Dainotti, MG; D'Elia, V; De Martino, D; De Pasquale, M; Del Monte, E; Della Valle, M; Drago, A; Evangelista, Y; Feroci, M; Finelli, F; Fiorini, M; Fynbo, J; Gal-Yam, A; Gendre, B; Ghisellini, G; Grado, A; Guidorzi, C; Hafizi, M; Hanlon, L; Hjorth, J; Izzo, L; Kiss, L; Kumar, P; Kuvvetli, I; Lavagna, M; Li, T; Longo, F; Lyutikov, M; Maio, U; Maiorano, E; Malcovati, P; Malesani, D; Margutti, R; Martin-Carrillo, A; Masetti, N; McBreen, S; Mignani, R; Morgante, G; Mundell, C; Nargaard-Nielsen, HU; Nicastro, L; Palazzi, E; Paltani, S; Panessa, F; Pareschi, G; Pe'er, A; Penacchioni, AV; Pian, E; Piedipalumbo, E; Piran, T; Rauw, G; Razzano, M; Read, A; Rezzolla, L; Romano, P; Ruffini, R; Savaglio, S; Sguera, V; Schady, P; Skidmore, W; Song, L; Stanway, E; Starling, R; Topinka, M; Troja, E; van Putten, M; Vanzella, E; Vercellone, S; Wilson-Hodge, C; Yonetoku, D; Zampa, G; Zampa, N; Zhang, B; Zhang, BB; Zhang, S; Zhang, SN; Antonelli, A; Bianco, F; Boci, S; Boer, M; Botticella, MT; Boulade, O; Butler, C; Campana, S; Capitanio, F; Celotti, A; Chen, Y; Colpi, M; Comastri, A; Cuby, JG; Dadina, M; De Luca, A; Dong, YW; Ettori, S; G; hi, P; Geza, E; Greiner, J; Guiriec, S; Harms, J; Hernanz, M; Hornstrup, A; Hutchinson, I; Israel, G; Jonker, P; Kaneko, Y; Kawai, N; Wiersema, K; Korpela, S; Lebrun, V; Lu, F; MacFadyen, A; Malaguti, G; Maraschi, L; Mel; ri, A; Modjaz, M; Morris, D; Omodei, N; Paizis, A; Pata, P; Petrosian, V; Rachevski, A; Rhoads, J; Ryde, F; Sabau-Graziati, L; Shigehiro, N; Sims, M; Soomin, J; Szecsi, D; Urata, Y; Uslenghi, M; Valenziano, L; Vianello, G; Vojtech, S; Watson, D; Zicha, J; Song LM(宋黎明)
2018
Source PublicationADVANCES IN SPACE RESEARCH
ISSN0273-1177
EISSN1879-1948
Volume62Issue:1Pages:191-244
SubtypeArticle
AbstractTHESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1 sr) with 0.5-1 arcmin localization, an energy band extending from several MeV down to 0.3 keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7 m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing the main open issues in cosmology such as, e.g., star formation rate and metallicity evolution of the inter-stellar and intra-galactic medium up to redshift similar to 10, signatures of Pop III stars, sources and physics of re-ionization, and the faint end of the galaxy luminosity function. In addition, it will provide unprecedented capability to monitor the X-ray variable sky, thus detecting, localizing, and identifying the electromagnetic counterparts to sources of gravitational radiation, which may be routinely detected in the late '20s/early '30s by next generation facilities like aLIGO/ aVirgo, eLISA, KAGRA, and Einstein Telescope. THESEUS will also provide powerful synergies with the next generation of multi-wavelength observatories (e.g., LSST, ELT, SKA, CTA, ATHENA). (C) 2018 COSPAR. Published by Elsevier Ltd. All rights reserved.
KeywordGamma-ray: bursts Cosmology: observations Dark ages Re-ionization First stars
DOI10.1016/j.asr.2018.03.010
WOS KeywordGAMMA-RAY BURSTS ; NEUTRON-STAR MERGER ; MASSIVE SINGLE STARS ; 7 CANDIDATE GALAXIES ; SIMILAR-TO 6 ; X-RAY ; BLACK-HOLE ; LIGHT CURVES ; LUMINOSITY FUNCTION ; TIDAL DISRUPTION
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences
WOS SubjectAstronomy & Astrophysics ; Geosciences, Multidisciplinary ; Meteorology & Atmospheric Sciences
WOS IDWOS:000436889000016
ADS Bibcode2018AdSpR..62..191A
AXRIV CODE1710
inspireid1630449
Citation statistics
Cited Times:32[WOS]   [WOS Record]     [Related Records in WOS]
Cited Times:49 [INSPIRE]
Document Type期刊论文
Identifierhttp://ir.ihep.ac.cn/handle/311005/286078
Collection多学科研究中心
粒子天体物理中心
Affiliation中国科学院高能物理研究所
First Author AffilicationInstitute of High Energy
Recommended Citation
GB/T 7714
Amati, L,O'Brien, P,Gotz, D,et al. The THESEUS space mission concept: science case, design and expected performances[J]. ADVANCES IN SPACE RESEARCH,2018,62(1):191-244.
APA Amati, L.,O'Brien, P.,Gotz, D.,Bozzo, E.,Tenzer, C.,...&宋黎明.(2018).The THESEUS space mission concept: science case, design and expected performances.ADVANCES IN SPACE RESEARCH,62(1),191-244.
MLA Amati, L,et al."The THESEUS space mission concept: science case, design and expected performances".ADVANCES IN SPACE RESEARCH 62.1(2018):191-244.
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