{
  "id": "2007.03715",
  "version": "v1",
  "published": "2020-07-07T18:08:25.000Z",
  "updated": "2020-07-07T18:08:25.000Z",
  "title": "Discovery of the optical afterglow and host galaxy of short GRB181123B at $z =1.754$: Implications for Delay Time Distributions",
  "authors": [
    "K. Paterson",
    "W. Fong",
    "A. Nugent",
    "A. Rouco Escorial",
    "J. Leja",
    "T. Laskar",
    "R. Chornock",
    "A. A. Miller",
    "J. Scharwächter",
    "S. B. Cenko",
    "D. Perley",
    "N. R. Tanvir",
    "A. Levan",
    "A. Cucchiara",
    "B. E. Cobb",
    "K. De",
    "E. Berger",
    "G. Terreran",
    "K. D. Alexander",
    "M. Nicholl",
    "P. K. Blanchard",
    "D. Cornish"
  ],
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "We present the discovery of the optical afterglow and host galaxy of the {\\it Swift} short-duration gamma-ray burst, GRB\\,181123B. Observations with Gemini-North starting at $\\approx 9.1$~hr after the burst reveal a faint optical afterglow with $i\\approx25.1$~mag, at an angular offset of 0.59 $\\pm$ 0.16$''$ from its host galaxy. Using $grizYJHK$ observations, we measure a photometric redshift of the host galaxy of $z = 1.77^{+0.30}_{-0.17}$. From a combination of Gemini and Keck spectroscopy of the host galaxy spanning 4500-18000~\\AA , we detect a single emission line at 13390~\\AA, inferred as H$\\beta$ at $z = 1.754 \\pm 0.001$ and corroborating the photometric redshift. The host galaxy properties of GRB\\,181123B are typical to those of other SGRB hosts, with an inferred stellar mass of $\\approx 1.7 \\times 10^{10}\\,M_{\\odot}$, mass-weighted age of $\\approx 0.9$~Gyr and optical luminosity of $\\approx 0.9L^{*}$. At $z=1.754$, GRB\\,181123B is the most distant secure SGRB with an optical afterglow detection, and one of only three at $z>1.5$. Motivated by a growing number of high-$z$ SGRBs, we explore the effects of a missing $z>1.5$ SGRB population among the current {\\it Swift} sample on delay time distribution models. We find that log-normal models with mean delay times of $\\approx 4-6$~Gyr are consistent with the observed distribution, but can be ruled out to $95\\%$ confidence with an additional $\\approx1-5$~{\\it Swift} SGRBs recovered at $z>1.5$. In contrast, power-law models with $\\propto$ $t^{-1}$ are consistent with the redshift distribution and can accommodate up to $\\approx30$ SGRBs at these redshifts. Under this model, we predict that $\\approx 1/3$ of the current {\\it Swift} population of SGRBs is at $z>1$. The future discovery or recovery of existing high-$z$ SGRBs will provide significant discriminating power on their delay time distributions, and thus their formation channels.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2020-07-07T18:08:25.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "optical afterglow",
      "short grb181123b",
      "delay time distribution models",
      "implications",
      "photometric redshift"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}