4.7 Article

Short GRB Host Galaxies. I. Photometric and Spectroscopic Catalogs, Host Associations, and Galactocentric Offsets

Journal

ASTROPHYSICAL JOURNAL
Volume 940, Issue 1, Pages -

Publisher

IOP Publishing Ltd
DOI: 10.3847/1538-4357/ac91d0

Keywords

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Funding

  1. National Science Foundation [AST-1909796, AST-1944985, AST-2047919, AST-1814782, AST-1909358]
  2. David and Lucile Packard Foundation
  3. Alfred P. Sloan Foundation
  4. Research Corporation for Science Advancement through Cottrell Scholar Award [28284]
  5. Henry Luce Foundation through a Graduate Fellowship in Physics and Astronomy
  6. National Science Foundation Graduate Research Fellowship [DGE-1842165]
  7. European Research Council (ERC) under the European Unions Horizon 2020 research and innovation program [725246, 948381]
  8. Alan Turing Institute
  9. NASA [NAS 526555]
  10. Northwestern University
  11. Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA)
  12. W. M. Keck Foundation
  13. NASA
  14. [14685]
  15. [13830]
  16. [14237]
  17. [14357]

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We present a comprehensive optical and near-infrared census of 90 short gamma-ray bursts (GRBs) discovered between 2005 and 2021. This provides detailed information about the host galaxies and properties, enriching our understanding of short GRBs.
We present a comprehensive optical and near-infrared census of the fields of 90 short gamma-ray bursts (GRBs) discovered in 2005-2021, constituting all short GRBs for which host galaxy associations are feasible (approximate to 60% of the total Swift short GRB population). We contribute 274 new multi-band imaging observations across 58 distinct GRBs and 26 spectra of their host galaxies. Supplemented by literature and archival survey data, the catalog contains 542 photometric and 42 spectroscopic data sets. The photometric catalog reaches 3 sigma depths of greater than or similar to 24-27 mag and greater than or similar to 23-26 mag for the optical and near-infrared bands, respectively. We identify host galaxies for 84 bursts, in which the most robust associations make up 56% (50/90) of events, while only a small fraction, 6.7%, have inconclusive host associations. Based on new spectroscopy, we determine 18 host spectroscopic redshifts with a range of z approximate to 0.15-1.5 and find that approximate to 23%-41% of Swift short GRBs originate from z > 1. We also present the galactocentric offset catalog for 84 short GRBs. Taking into account the large range of individual measurement uncertainties, we find a median of projected offset of approximate to 7.7 kpc, for which the bursts with the most robust associations have a smaller median of approximate to 4.8 kpc. Our catalog captures more high-redshift and low-luminosity hosts, and more highly offset bursts than previously found, thereby diversifying the population of known short GRB hosts and properties. In terms of locations and host luminosities, the populations of short GRBs with and without detectable extended emission are statistically indistinguishable. This suggests that they arise from the same progenitors, or from multiple progenitors, which form and evolve in similar environments. All of the data products are available on the Broadband Repository for Investigating Gamma-Ray Burst Host Traits website.

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