{
  "id": "2408.10983",
  "version": "v1",
  "published": "2024-08-20T16:22:06.000Z",
  "updated": "2024-08-20T16:22:06.000Z",
  "title": "Search for GeV gamma-ray emission from SPT-CL J2012-5649 with six years of DAMPE data",
  "authors": [
    "Siddhant Manna",
    "Shantanu Desai"
  ],
  "comment": "7 pages, 3 figures",
  "categories": [
    "astro-ph.HE",
    "astro-ph.CO"
  ],
  "abstract": "We search for gamma-ray emission from the galaxy cluster SPT-CL J2012-5649 in the energy range from 3 GeV to 1 TeV using the DArk Matter Particle Explorer (DAMPE) telescope. For our analysis, we use three different templates: point source, radial disk and radial Gaussian. We do not detect a signal with significance $>3\\sigma$ for any of these templates at any location with $R_{200}$ of the cluster center. We obtain 95\\% c.l. upper limit on the energy flux between $\\sim 10^{-6}$ and $10^{-4} \\rm{MeV~cm^{-2}~s^{-1}}$ depending on the energy range. These upper limits are consistent with the a non-zero flux detected by Fermi-LAT (at $6\\sigma$ significance) for this cluster. This work represents the first proof of principle search for gamma-ray emission from a single galaxy cluster using DAMPE data.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2024-08-20T16:22:06.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "gev gamma-ray emission",
      "dampe data",
      "upper limit",
      "energy range",
      "dark matter particle explorer"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 7,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}