{ "id": "1010.4167", "version": "v1", "published": "2010-10-20T11:49:23.000Z", "updated": "2010-10-20T11:49:23.000Z", "title": "X-ray pulsations from the radio-quiet gamma-ray pulsar in CTA 1", "authors": [ "P. A. Caraveo", "A. De Luca", "M. Marelli", "G. F. Bignami", "P. S. Ray", "P. M. Saz-Parkinson", "G. Kanbach" ], "comment": "19 pages, 4 figures. Accepted for publication in ApJ Letters", "categories": [ "astro-ph.HE" ], "abstract": "Prompted by the Fermi LAT discovery of a radio-quiet gamma-ray pulsar inside the CTA 1 supernova remnant, we obtained a 130 ks XMM-Newton observation to assess the timing behavior of this pulsar. Exploiting both the unprecedented photon harvest and the contemporary Fermi LAT timing measurements, a 4.7 sigma single peak pulsation is detected, making PSR J0007+7303 the second example, after Geminga, of a radio-quiet gamma-ray pulsar also seen to pulsate in X-rays. Phase-resolved spectroscopy shows that the off-pulse portion of the light curve is dominated by a power-law, non-thermal spectrum, while the X-ray peak emission appears to be mainly of thermal origin, probably from a polar cap heated by magnetospheric return currents, pointing to a hot spot varying throughout the pulsar rotation.", "revisions": [ { "version": "v1", "updated": "2010-10-20T11:49:23.000Z" } ], "analyses": { "keywords": [ "x-ray pulsations", "sigma single peak pulsation", "contemporary fermi lat timing measurements", "x-ray peak emission appears", "radio-quiet gamma-ray pulsar inside" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/2041-8205/725/1/L6", "journal": "The Astrophysical Journal", "year": 2010, "month": "Dec", "volume": 725, "number": 1 }, "note": { "typesetting": "TeX", "pages": 19, "language": "en", "license": "arXiv", "status": "editable", "inspire": 873513, "adsabs": "2010ApJ...725L...6C" } } }