{
  "id": "1404.1532",
  "version": "v2",
  "published": "2014-04-06T00:24:58.000Z",
  "updated": "2014-05-30T23:25:49.000Z",
  "title": "High-energy pulsations and phase-resolved spectroscopy of PSR J1741-2054",
  "authors": [
    "M. Marelli",
    "A. Belfiore",
    "P. Saz Parkinson",
    "P. Caraveo",
    "A. De Luca",
    "C. Sarazin",
    "D. Salvetti",
    "G. R. Sivakoff",
    "F. Camilo"
  ],
  "comment": "12 pages, 4 figures, accepted by the Astrophysical Journal",
  "journal": "Marelli et al. 2014, ApJ, 790, 51",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "We report the results of a deep XMM-Newton observation of the radio-faint $\\gamma$-ray pulsar J1741-2054 and its nebula together with the analysis of 5 years of Fermi LAT data. The X-ray spectrum of the pulsar is consistent with an absorbed power law plus a blackbody, originating at least partly from the neutron star cooling. The nebular emission is consistent with that of a synchrotron pulsar wind nebula, with hints of spatial spectral variation. We extended the available Fermi LAT ephemeris and folded the $\\gamma$-ray and X-ray data. We detected X-ray pulsations from the neutron star: both the thermal and non-thermal components are about 35-40% pulsed, with phase-aligned maxima. A sinusoid fits the thermal folded profile well. A 10-bin phase-resolved analysis shows softening of the non-thermal spectrum during the on-pulse phases. The radio, X-ray and $\\gamma$-ray light curves are single-peaked, not phase-aligned, with the X-ray peak trailing the $\\gamma$-ray peak by over half a rotation. Spectral considerations suggest that the most probable pulsar distance is in the 0.3-1.0 kpc range.",
  "revisions": [
    {
      "version": "v2",
      "updated": "2014-05-30T23:25:49.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "high-energy pulsations",
      "phase-resolved spectroscopy",
      "synchrotron pulsar wind nebula",
      "neutron star",
      "absorbed power law plus"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1088/0004-637X/790/1/51",
      "journal": "The Astrophysical Journal",
      "year": 2014,
      "month": "Jul",
      "volume": 790,
      "number": 1,
      "pages": 51
    },
    "note": {
      "typesetting": "TeX",
      "pages": 12,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1288828,
      "adsabs": "2014ApJ...790...51M"
    }
  }
}