{ "id": "2205.06696", "version": "v1", "published": "2022-05-13T15:05:17.000Z", "updated": "2022-05-13T15:05:17.000Z", "title": "Black Hole Spin Measurements Based on a Thin Disc Model with Finite Thickness I. An example study of MCG-06-30-15", "authors": [ "Jiachen Jiang", "Askar B. Abdikamalov", "Cosimo Bambi", "Christopher S. Reynolds" ], "comment": "15 pages, 14 figures, accepted for publication in MNRAS", "categories": [ "astro-ph.HE" ], "abstract": "We present a re-analysis of the XMM-Newton and NuSTAR observing campaign for the well-studied, X-ray-bright AGN MCG-06-30-15. In particular, we consider a disc model with finite thickness. By fitting the disc reflection spectra in the data, we obtain a black hole spin of 0.87--0.99 (90\\% confidence range) after taking the thickness of the disc into consideration. Spectral models with a grid of mass accretion rate from 0 to $30\\%\\dot{M}_{\\rm Edd}$ are calculated for MCG-06-30-15. This result is obtained by considering a free disc reflection fraction parameter $f_{\\rm refl}$ and is consistent with previous measurements based on razor-thin disc models. Besides, an isotropic, point-like geometry, i.e. the `lamppost' geometry, is assumed for the corona in our model. We find that such a geometry overestimates $f_{\\rm refl}$ in the data. Therefore, thin disc models with consistent `lamppost' values of $f_{\\rm refl}$ provide a worse fit than ones with a free $f_{\\rm refl}$ parameter. We discuss possible reasons for the discrepancy between the observed and theoretical values of $f_{\\rm refl}$ at the end of the paper. Modifications for the over-simplified lamppost model might be needed when the thickness of the thin disc is considered in future work.", "revisions": [ { "version": "v1", "updated": "2022-05-13T15:05:17.000Z" } ], "analyses": { "keywords": [ "black hole spin measurements", "thin disc model", "finite thickness", "example study", "free disc reflection fraction parameter" ], "note": { "typesetting": "TeX", "pages": 15, "language": "en", "license": "arXiv", "status": "editable" } } }