Spectroscopy of the short-hard GRB 130603B
A. de Ugarte PostigoDark Cosmology Centre, Niels Bohr Institute, Juliane Maries Vej 30, 2100 Copenhagen Ø, DenmarkC. C. ThöneInstituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, 18008 Granada, SpainA. RowlinsonAstronomical Institute “Anton Pannekoek”, University of Amsterdam, Postbus 94249, 1090 GE Amsterdam, The NetherlandsR. García-BenitoInstituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, 18008 Granada, SpainA. J. LevanDepartment of Physics, University of Warwick, Coventry, CV4 7AL, UKJ. GorosabelUnidad Asociada Grupo Ciencia Planetarias UPV/EHU-IAA/CSIC, Departamento de Física Aplicada I, E.T.S. Ingeniería, Universidad del País-Vasco UPV/EHU, Alameda de Urquijo s/n, 48013 Bilbao, SpainP. GoldoniInstitut de Recherche sur les Lois Fondamentales de l'UniversS. SchulzePontificia Universidad Católica de Chile, Departamento de Astronomía y Astrofísica, Casilla 306, 22 Santiago, ChileTayyaba ZafarEuropean Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching, GermanyK. WiersemaDepartment of Physics and Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UKR. Sánchez-RamírezInstituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, 18008 Granada, SpainA. MelandriINAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate, ItalyP. D’AvanzoINAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate, ItalyS. R. OatesMullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UKV. D’EliaASI – Science Data Center, via Galileo Galilei, 00044 Frascati, ItalyM. de PasqualeMullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UKT. KrühlerDark Cosmology Centre, Niels Bohr Institute, Juliane Maries Vej 30, 2100 Copenhagen Ø, DenmarkA. J. van der HorstAstronomical Institute “Anton Pannekoek”, University of Amsterdam, Postbus 94249, 1090 GE Amsterdam, The NetherlandsD. XuD. WatsonS. PiranomonteINAF-Osservatorio Astronomico di Roma, via Frascati 33, 00040 Monte Porzio Catone, Rome, ItalyS. D. VerganiBrera Astronomical ObservatoryB. Milvang‐JensenL. KaperAstronomical Institute “Anton Pannekoek”, University of Amsterdam, Postbus 94249, 1090 GE Amsterdam, The NetherlandsD. MalesaniJ. P. U. FynboZ. CanoCentre for Astrophysics and Cosmology, Science Institute, University of Iceland, 150 Reykjavik, IcelandS. CovinoINAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate, ItalyH. FloresLaboratoire GEPI, Observatoire de Paris, CNRS-UMR8111, Univ. Paris Diderot, 5 place Jules Janssen, 92195 Meudon, FranceS. GreissDepartment of Physics, University of Warwick, Coventry, CV4 7AL, UKF. HammerUniversité Paris CitéO. E. HartoogAstronomical Institute “Anton Pannekoek”, University of Amsterdam, Postbus 94249, 1090 GE Amsterdam, The NetherlandsS. HellmichC. HeuserDr. Karl Remeis-Observatory & ECAP, Astronomical Institute, Friedrich-Alexander University, Erlangen-Nuremberg, Sternwartstr. 7, 96049 Bamberg, GermanyJ. HjorthP. JakobssonCentre for Astrophysics and Cosmology, Science Institute, University of Iceland, 150 Reykjavik, IcelandS. MottolaMartin SparreJ. SollermanDepartment of Astronomy, AlbaNova Science Center, Stockholm University, 106 91 Stockholm, SwedenG. TagliaferriINAF – Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate, ItalyN. R. TanvirDepartment of Physics and Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UKM. VestergaardDark Cosmology Centre, Niels Bohr Institute, Juliane Maries Vej 30, 2100 Copenhagen Ø, DenmarkR. A. M. J. WijersAstronomical Institute “Anton Pannekoek”, University of Amsterdam, Postbus 94249, 1090 GE Amsterdam, The Netherlands
2013en
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Context. Short duration gamma-ray bursts (SGRBs) are thought to be related to the violent merger of compact objects, such as neutron stars or black holes, which makes them promising sources of gravitational waves. The detection of a “kilonova”-likesignature associated to the Swift-detected GRB 130603B has suggested that this event is the result of a compact object merger.
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