{ "id": "1001.2407", "version": "v1", "published": "2010-01-14T10:45:42.000Z", "updated": "2010-01-14T10:45:42.000Z", "title": "New results with Swift on Supergiant Fast X-ray Transients", "authors": [ "L. Sidoli", "P. Romano", "L. Ducci", "A. Paizis", "S. Vercellone", "G. Cusumano", "V. La Parola", "V. Mangano", "J. A. Kennea", "D. N. Burrows", "H. A. Krimm", "N. Gehrels", "V. Sguera", "A. Bazzano" ], "comment": "Accepted for publication on PoS (contribution PoS(extremesky2009)059), proceedings of \"The Extreme sky: Sampling the Universe above 10 keV\", held in Otranto (Italy) in October 2009", "categories": [ "astro-ph.HE" ], "abstract": "We report here on the most recent results obtained on a new class of High Mass X-ray Binaries, the Supergiant Fast X-ray Transients. Since October 2007, we have been performing a monitoring campaign with Swift of four SFXTs (IGRJ17544-2916, XTEJ1739-302, IGRJ16479-4514 and the X-ray pulsar AXJ1841.0-0536) for about 1-2 ks, 2-3 times per week, allowing us to derive the previously unknown long term properties of this new class of sources (their duty cycles, spectral properties in outbursts and out-of-outbursts, temporal behaviour). We also report here on additional Swift observations of two SFXTs which are not part of the monitoring: IGRJ18483-0311 (observed with Swift/XRT during a whole orbital cycle) and SAXJ1818.6-1703 (observed for the first time simultaneously in the energy range 0.3-100 keV during a bright flare).", "revisions": [ { "version": "v1", "updated": "2010-01-14T10:45:42.000Z" } ], "analyses": { "keywords": [ "supergiant fast x-ray transients", "high mass x-ray binaries", "unknown long term properties", "additional swift observations", "x-ray pulsar axj1841" ], "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 842816, "adsabs": "2010arXiv1001.2407S" } } }