{
  "id": "1309.1015",
  "version": "v1",
  "published": "2013-09-04T12:56:51.000Z",
  "updated": "2013-09-04T12:56:51.000Z",
  "title": "Statistical analysis of the prompt and afterglow emission of the three groups of gamma-ray bursts",
  "authors": [
    "J. Kóbori",
    "Z. Bagoly",
    "L. G. Balázs",
    "I. Horváth"
  ],
  "comment": "7th Huntsville Gamma-Ray Burst Symposium, GRB 2013: paper 27 in eConf Proceedings C1304143",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "We investigated the main prompt and afterglow emission parameters of gamma-ray bursts detected by the Burst Alert Telescope (BAT) and X-Ray Telescope installed on the Swift satellite. Our aim was to look for differences or connections between the different types of gamma-ray bursts, so we compared the BAT fluences, 1-sec peak photon fluxes, photon indices, XRT early fluxes, initial temporal decay and spectral indices. We found that there might be a connection between the XRT initial decay index and XRT early flux/BAT photon index. Using statistical tools we also determined that beside the duration and hardness ratios, the means of the \\gamma- and X-ray--fluences and the \\gamma-ray photon index differ significantly between the three types of bursts.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2013-09-04T12:56:51.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "gamma-ray bursts",
      "statistical analysis",
      "xrt early flux/bat photon index",
      "xrt initial decay index",
      "afterglow emission parameters"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1252679,
      "adsabs": "2013arXiv1309.1015K"
    }
  }
}