{ "id": "1106.2140", "version": "v1", "published": "2011-06-10T18:30:04.000Z", "updated": "2011-06-10T18:30:04.000Z", "title": "Is Calvera a Gamma-ray Pulsar?", "authors": [ "J. P. Halpern" ], "comment": "5 pages, 4 figures, to appear in The Astrophysical Journal Letters", "categories": [ "astro-ph.HE" ], "abstract": "Originally selected as a neutron star (NS) candidate in the ROSAT All-Sky Survey, 1RXS J141256.0+792204 (\"Calvera\") was discovered to be a 59 ms X-ray pulsar in a pair of XMM-Newton observations (Zane et al. 2011). Surprisingly, their claimed detection of this pulsar in Fermi gamma-ray data requires no period derivative, severely restricting its dipole magnetic field strength, spin-down luminosity, and distance to small values. This implies that the cooling age of Calvera is much younger than its characteristic spin-down age. If so, it could be a mildly recycled pulsar, or the first \"orphaned\" central compact object (CCO). Here we show that the published Fermi ephemeris fails to align the pulse phases of the two X-ray observations with each other, which indicates that the Fermi detection is almost certainly spurious. Analysis of additional Fermi data also does not confirm the gamma-ray detection. This leaves the spin-down rate of Calvera less constrained, and its place among the families of NSs uncertain. It could still be either a normal pulsar, a mildly recycled pulsar, or an orphaned CCO.", "revisions": [ { "version": "v1", "updated": "2011-06-10T18:30:04.000Z" } ], "analyses": { "keywords": [ "gamma-ray pulsar", "dipole magnetic field strength", "mildly recycled pulsar", "rosat all-sky survey", "ms x-ray pulsar" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/2041-8205/736/1/L3", "journal": "The Astrophysical Journal", "year": 2011, "month": "Jul", "volume": 736, "number": 1 }, "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable", "inspire": 913323, "adsabs": "2011ApJ...736L...3H" } } }