GRB hosts through cosmic time: VLT/X-Shooter emission-line spectroscopy of 96 γ-ray-burst-selected galaxies at 0.1 <z < 3.6
- Krühler, T.
- Malesani, D.
- Fynbo, J. P. U.
- Hartoog, O. E.
- Hjorth, J.
- Jakobsson, P.
- Perley, D. A.
- Rossi, A.
- Schady, P.
- Schulze, S.
- Tanvir, N. R.
- Vergani, S. D.
- Wiersema, K.
- Afonso, P. M. J.
- Bolmer, J.
- Cano, Z.
- Covino, S.
- D’elia, V.
- de Ugarte Postigo, A.
- Filgas, R.
- Friis, M.
- Graham, J. F.
- Greiner, J.
- Goldoni, P.
- Gomboc, A.
- Hammer, F.
- Japelj, J.
- Kann, D. A.
- Kaper, L.
- Klose, S.
- Levan, A. J.
- Leloudas, G.
- Milvang-Jensen, B.
- Nicuesa Guelbenzu, A.
- Palazzi, E.
- Pian, E.
- Piranomonte, S.
- Sánchez-Ramírez, R.
- Savaglio, S.
- Selsing, J.
- Tagliaferri, G.
- Vreeswijk, P. M.
- Watson, D. J.
- Xu, D.
DOIAbstract
International audienceWe present data and initial results from VLT/X-Shooter emission-line spectroscopy of 96 galaxies selected by long γ-ray bursts (GRBs) at 0.1 2 by ~0.4 dex. These properties of GRB hosts and their evolution with redshift can be understood in a cosmological context of star-forming galaxies and a picture in which the hosts’ properties at low redshift are influenced by the tendency of GRBs to avoid the most metal-rich environments
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