机译:The low-extinction afterglow in the solar-metallicity host galaxy of γ -ray burst 110918A
Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstra?e 1, 85748 Garching, Germany;
Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen, Denmark;
Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía S/n, 18008 Granada, SpainUniversity of Leicester, Department of Physics and Astronomy, University Road, Leicester, LE1 7RH, United KingdomUniversità Degli Studi di Milano-Bicocca, Piazza della Scienza 3, 20126 Milano, ItalyHarvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, United StatesDepartment of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802, United StatesThüringer Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenburg, GermanyDepartment of Physics, University of Warwick, Coventry CV4 7AL, United Kingdom;
Galaxies: abundances; Galaxies: photometry; Galaxies: star formation; Gamma-ray burst: general; Gamma-ray burst: individual: 110918A; ISM: general;