{
  "id": "1505.01368",
  "version": "v1",
  "published": "2015-05-06T13:59:48.000Z",
  "updated": "2015-05-06T13:59:48.000Z",
  "title": "SOUSA's Swift Supernova Siblings",
  "authors": [
    "Peter J. Brown"
  ],
  "comment": "Submitted to Proceedings of Science for the \"10 Years of Swift\" Meeting held in Rome in December 2014",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "Swift has observed over three hundred supernovae in its first ten years. Photometry from the Ultra-Violet Optical Telescope (UVOT) is being compiled in the Swift Optical/Ultraviolet Supernovae Archive (SOUSA). The diversity of supernovae leads to a wide dynamic range of intrinsic properties. The intrinsic UV brightness of supernovae as a function of type and epoch allows one to understand the distance ranges at which Swift can reliably detect supernovae. The large Swift sample also includes supernovae from the same galaxy as other Swift supernovae. Through the first ten years, these families include 34 supernovae from 16 host galaxies (two galaxies have each hosted three Swift supernovae).",
  "revisions": [
    {
      "version": "v1",
      "updated": "2015-05-06T13:59:48.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "sousas swift supernova siblings",
      "large swift sample",
      "wide dynamic range",
      "intrinsic uv brightness",
      "swift optical/ultraviolet supernovae archive"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1367049
    }
  }
}