{ "id": "1209.3883", "version": "v1", "published": "2012-09-18T09:11:03.000Z", "updated": "2012-09-18T09:11:03.000Z", "title": "Confirming the 115.5-day periodicity in the X-ray light curve of ULX NGC 5408 X-1", "authors": [ "Xu Han", "Tao An", "Jun-Yi Wang", "Ji-Ming Lin", "Ming-Jie Xie", "Hai-Guang Xu", "Xiao-Yu Hong", "Sandor Frey" ], "comment": "6 pages, 2 figures, submitted to Research in Astronomy and Astrophysics (RAA)", "categories": [ "astro-ph.HE", "astro-ph.SR" ], "abstract": "The Swift/XRT light curve of the ultraluminous X-ray (ULX) source NGC 5408 X-1 was re-analyzed with two new numerical approaches, Weighted Wavelet $Z$-transform (WWZ) and CLEANest, that are different from previous studies. Both techniques detected a prominent periodicity with a time scale of $115.5\\pm1.5$ days, in excellent agreement with the detection of the same periodicity first reported by Strohmayer (2009). Monte Carlo simulation was employed to test the statisiticak confidence of the 115.5-day periodicity, yielding a statistical significance of $> 99.98%$ (or $>3.8\\sigma$). The robust detection of the 115.5-day quasi-periodic oscillations (QPOs), if it is due to the orbital motion of the binary, would infer a mass of a few thousand $M_\\odot$ for the central black hole, implying an intermediate-mass black hole in NGC 5408 X-1.", "revisions": [ { "version": "v1", "updated": "2012-09-18T09:11:03.000Z" } ], "analyses": { "keywords": [ "x-ray light curve", "ulx ngc", "periodicity", "swift/xrt light curve", "central black hole" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/1674-4527/12/12/001", "journal": "Research in Astronomy and Astrophysics", "year": 2012, "month": "Dec", "volume": 12, "pages": 1597 }, "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1186349, "adsabs": "2012RAA....12.1597H" } } }