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Exploration of the high-redshift universe enabled by THESEUS |
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| Authors: | Tanvir N. R. Le Floc’h E. Christensen L. Caruana J. Salvaterra R. Ghirlanda G. Ciardi B. Maio U. D’Odorico V. Piedipalumbo E. Campana S. Noterdaeme P. Graziani L. Amati L. Bagoly Z. Balázs L. G. Basa S. Behar E. De Cia A. Valle M. Della De Pasquale M. Frontera F. Gomboc A. Götz D. Horvath I. Hudec R. Mereghetti S. O’Brien P. T. Osborne J. P. Paltani S. Rosati P. Sergijenko O. Stanway E. R. Szécsi D. Tot́h L. V. Urata Y. Vergani S. Zane S. |
| Affiliation: | 1.School of Physics and Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UK ;2.AIM, CEA-Irfu/DAp, CNRS, Université Paris-Saclay, F-91191, Gif-sur-Yvette, France ;3.Niels Bohr Institute, University of Copenhagen, Jagtvej 128, 2200, Copenhagen N, Denmark ;4.Department of Physics and Institute of Space Sciences and Astronomy, University of Malta, Msida, MSD 2080, Malta ;5.INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica, via Alfonso Corti 12, 20133, Milano, Italy ;6.INAF-Osservatorio Astronomico di Brera, Via Bianchi 46, I-23807, Merate (LC), Italy ;7.Max Planck Institute for Astrophysics, Karl-Schwarzschild-Str. 1, 85741, Garching, Germany ;8.INAF-Observatory of Trieste, via G. Tiepolo 11, 34143, Trieste, Italy ;9.Dipartimento di Fisica, Università degli Studi di Napoli Federico II, 80126, Naples, Italy ;10.I.N.F.N., Sez. di Napoli, Compl. Univ. Monte S. Angelo, via Cinthia, 80126, Napoli, Italy ;11.Institut d’Astrophysique de Paris, CNRS-SU, UMR 7095, 98bis bd Arago, 75014, Paris, France ;12.Dipartimento di Fisica, “Sapienza” Università di Roma, Piazzale Aldo Moro 5, 00185, Roma, Italy ;13.INAF/OAS-Bologna, via P. Gobetti 101, I-40129, Bologna, Italy ;14.E?v?s University, H-1117, Budapest, Hungary ;15.CSFK Konkoly Observatory, Budapest, Hungary ;16.Department of Astronomy, E?v?s University, Budapest, Hungary ;17.CNRS, CNES, LAM, Aix Marseille Universite, Marseille, France ;18.Department of Physics, Technion, Israel ;19.Department of Astronomy, University of Geneva, Chemin Pegasi 51, 1290, Versoix, Switzerland ;20.INAF-Capodimonte Observatory, Salita Moiariello 16, 80131, Napoli, Italy ;21.Department of Astronomy and Space Sciences, Istanbul University, Beyaz?t, 34119, Istanbul, Turkey ;22.Dipartimento di Fisica e Scienze della Terra, Università di Ferrara, Via Saragat 1, I-44122, Ferrara, Italy ;23.Center for Astrophysics and Cosmology, University of Nova Gorica, Vipavska 13, 5000, Nova Gorica, Slovenia ;24.IRFU/Département d’Astrophysique, CEA, Université Paris-Saclay, F-91191, Gif-sur-Yvette, France ;25.University of Public Service, Budapest, Hungary ;26.Faculty of Electrical Engineering, Czech Technical University in Prague, Prague, Czech Republic ;27.Astronomical Institute, Czech Academy of Sciences, Ondrejov, Czech Republic ;28.Kazan Federal University, Kazan, Russian Federation ;29.INAF / IASF-Milano, via A. Corti 12, I-20133, Milano, Italy ;30.School of Physics and Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UK ;31.Department of Physics and Earth Sciences, University of Ferrara, Ferrara, Italy ;32.Astronomical Observatory of Taras Shevchenko, National University of Kyiv, Observatorna str., 3, Kyiv, 04053, Ukraine ;33.Main Astronomical Observatory of the National Academy of Sciences of Ukraine, Zabolotnoho str., 27, Kyiv, 03680, Ukraine ;34.Physical Sciences, University of Warwick, Gibbet Hill Road, Coventry, CV4 7AL, UK ;35.Institute of Astronomy, Nicolaus Copernicus University, 87-100, Toruń, Poland ;36.I. Physikalisches Institut, Universit?t zu K?ln, D-50937, Cologne, Germany ;37.Department of Astronomy, E?tv?s Loránd University, Pázmány Péter sétány 1/A, H-1117, Budapest, Hungary ;38.Institute of Astronomy, National Central University, Chung-Li, 32054, Taiwan ;39.CNRS, GEPI, Observatoire de Paris, PSL University, Place Jules Janssen, 92190, Meudon, France ;40.Mullard Space Science Laboratory, University College London, Holmbury St Mary, Dorking, RH56NT, UK ; |
| Abstract: | Experimental Astronomy - At peak, long-duration gamma-ray bursts are the most luminous sources of electromagnetic radiation known. Since their progenitors are massive stars, they provide a tracer... |
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