posted on 2019-06-25, 14:56authored byNR Tanvir, JPU Fynbo, ADU Postigo, J Japelj, K Wiersema, D Malesani, DA Perley, AJ Levan, J Selsing, SB Cenko, DA Kann, B Milvang-Jensen, E Berger, Z Cano, R Chornock, S Covino, A Cucchiara, V D'Elia, P Goldoni, A Gomboc, KE Heintz, J Hjorth, L Izzo, P Jakobsson, L Kaper, T Kruehler, T Laskar, M Myers, S Piranomonte, G Pugliese, R Sanchez-Ramirez, S Schulze, M Sparre, ER Stanway, G Tagliaferri, CC Thoene, S Vergani, PM Vreeswijk, RAMJ Wijers, D Watson, D Xu
Whether stars could have driven the reionization of the intergalactic medium depends critically
on the proportion of ionizing radiation that escapes the galaxies in which it is produced.
Spectroscopy of gamma-ray burst (GRB) afterglows can be used to estimate the opacity to
extreme ultraviolet (EUV) radiation along the lines-of-sight to the bursts. Assuming that
long-duration GRBs trace the locations of the massive stars dominating EUV production, the
average escape fraction of ionizing radiation can be calculated independently of galaxy size
or luminosity. Here we present a compilation of H I column density (NH I) measures for 140
GRBs in the range 1.6
Funding
Partly based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme IDs 280.D-5059, 081.A-0856, 082.A-0301, 083.A-0644, 091.A-0442, 100.D-0649, and 102.D-0662.
Partly based on observations made with the Nordic Optical Telescope, operated by the Nordic Optical Telescope Scientific Association at the Observatorio del Roque de los Muchachos, La Palma, Spain, of the Instituto de Astrofísica de Canarias, under programs 31-014, 32-010, 39-023, 48-005, and 51-504.
Partly based on observations made with the Gran Telescopio Canarias (GTC), installed in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofśica de Canarias, in the island of La Palma, Spain.
Partly based on observations made with the Italian Telescopio Nazionale Galileo (TNG) operated on the island of La Palma by the Fundación Galileo Galilei of the INAF (Istituto Nazionale di Astrofisica) at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias, under programs A26TAC_63 and A32TAC_5.
The WHT and its override programme (for 090715B: programme W09AN001, P.I. Curran; for 161017A: programme W/2017A/23, P.I. Levan) are operated on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. We thank A. Kamble, R. Starling, and P. Curran for their help with the 090715B observations, and Marie Hrudkova for executing the 161017A observations.
Partly based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina), and Ministério da Ciência, Tecnologia e Inovação (Brazil).
Partially
History
Citation
Monthly Notices of the Royal Astronomical Society, 2019, 483(4), pp. 5380–5408
Author affiliation
/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy
Version
VoR (Version of Record)
Published in
Monthly Notices of the Royal Astronomical Society
Publisher
Oxford University Press (OUP), Royal Astronomical Society