{
  "id": "0912.3847",
  "version": "v1",
  "published": "2009-12-19T01:28:49.000Z",
  "updated": "2009-12-19T01:28:49.000Z",
  "title": "Long-term Monitoring of Accreting Pulsars with Fermi GBM",
  "authors": [
    "Mark H. Finger",
    "Elif Beklen",
    "P. Narayana Bhat",
    "William S. Paciesas",
    "Valerie Connaughton",
    "David A. H. Buckley",
    "Ascension Camero-Arranz",
    "Malcolm J. Coe",
    "Peter Jenke",
    "Gottfried Kanbach",
    "Ignacio Negueruela",
    "Colleen A. Wilson-Hodge"
  ],
  "comment": "To appear in the proceedings of 2009 Fermi Symposium, eConf Proceedings C091122",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "Using the Gamma ray Burst Monitor (GBM) on Fermi we are monitoring accreting pulsar systems. We use the rates from GBM's 12 NaI detectors in the 8-50 keV range to detect and monitor pulsations with periods between 0.5 and 1000 seconds. After discussing our analysis approach we present results for individual sources from the first year of monitoring. Updated figures for these and other sources are available at http://gammaray.nsstc.nasa.gov/gbm/science/pulsars/ .",
  "revisions": [
    {
      "version": "v1",
      "updated": "2009-12-19T01:28:49.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "fermi gbm",
      "long-term monitoring",
      "gamma ray burst monitor",
      "nai detectors",
      "kev range"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 840772,
      "adsabs": "2009arXiv0912.3847F"
    }
  }
}