{ "id": "1608.06869", "version": "v1", "published": "2016-08-24T15:44:42.000Z", "updated": "2016-08-24T15:44:42.000Z", "title": "Improving the Flux Calibration in Reverberation Mapping by Spectral Fitting: Application to the Seyfert Galaxy MCG--6-30-15", "authors": [ "Chen Hu", "Jian-Min Wang", "Luis C. Ho", "Jin-Ming Bai", "Yan-Rong Li", "Pu Du", "Kai-Xing Lu" ], "comment": "8 pages, 6 figures, accepted for publication in The Astrophysical Journal", "categories": [ "astro-ph.GA" ], "abstract": "We propose a method for the flux calibration of reverberation mapping spectra based on accurate measurement of [O III] $\\lambda 5007$ emission by spectral fitting. The method can achieve better accuracy than the traditional method of van Groningen & Wanders (1992), allowing reverberation mapping measurements for object with variability amplitudes as low as $\\sim$ 5%. As a demonstration, we reanalyze the data of the Seyfert 1 galaxy MCG--6-30-15 taken from the 2008 campaign of the Lick AGN Monitoring Project, which previously failed to obtain a time lag for this weakly variable object owing to a relatively large flux calibration uncertainty. We detect a statistically significant rest-frame time lag of $6.38_{-2.69}^{+3.07}$ days between the H$\\beta$ and $V$-band light curves. Combining this lag with FWHM(H$\\beta$) = $1933\\pm81$ $\\rm km~s^{-1}$ and a virial coefficient of $f$ = 0.7, we derive a virial black hole mass of $3.26_{-1.40}^{+1.59}\\times10^6$ $M_{\\odot}$, which agrees well with previous estimates by other methods.", "revisions": [ { "version": "v1", "updated": "2016-08-24T15:44:42.000Z" } ], "analyses": { "keywords": [ "reverberation mapping", "spectral fitting", "seyfert galaxy", "relatively large flux calibration uncertainty", "application" ], "note": { "typesetting": "TeX", "pages": 8, "language": "en", "license": "arXiv", "status": "editable" } } }