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dc.contributor.authorBontà, Elena Dalla
dc.contributor.authorPeterson, Bradley M.
dc.contributor.authorBentz, Misty C.
dc.contributor.authorBrandt, W. N.
dc.contributor.authorCiroi, Stefano
dc.contributor.authorDe Rosa, Gisella
dc.contributor.authorFonseca Alvarez, Gloria
dc.contributor.authorGrier, Catherine J.
dc.contributor.authorHall, P. B.
dc.contributor.authorSantisteban, Juan V. Hernandez
dc.contributor.authorHo, Luis C.
dc.contributor.authorHomayouni, Y.
dc.contributor.authorHorne, Keith
dc.contributor.authorKochanek, C. S.
dc.contributor.authorLi, Jennifer I-Hsiu
dc.contributor.authorMorelli, Lorenzo
dc.contributor.authorPizzella, Alessandro
dc.contributor.authorPogge, R. W.
dc.contributor.authorSchneider, D. P.
dc.contributor.authorShen, Yue
dc.contributor.authorTrump, J. R.
dc.contributor.authorVestergaard, Marianne
dc.identifier.citationBontà , E D , Peterson , B M , Bentz , M C , Brandt , W N , Ciroi , S , De Rosa , G , Fonseca Alvarez , G , Grier , C J , Hall , P B , Santisteban , J V H , Ho , L C , Homayouni , Y , Horne , K , Kochanek , C S , Li , J I-H , Morelli , L , Pizzella , A , Pogge , R W , Schneider , D P , Shen , Y , Trump , J R & Vestergaard , M 2020 , ' The Sloan Digital Sky Survey Reverberation Mapping Project : estimating masses of black holes in quasars with single-epoch spectroscopy ' , Astrophysical Journal , vol. 903 , no. 2 , 112 .
dc.identifier.otherPURE: 270387278
dc.identifier.otherPURE UUID: fa92f4f1-6b85-42cb-a2a4-81e22350f3c2
dc.identifier.otherScopus: 85095509541
dc.identifier.otherORCID: /0000-0002-6733-5556/work/92775859
dc.identifier.otherWOS: 000588232100001
dc.descriptionFunding: JVHS and KH acknowledge support from UK STFC grant ST/R000824/1.en
dc.description.abstractIt is well known that reverberation mapping of active galactic nuclei (AGNs) reveals a relationship between AGN luminosity and the size of the broad-line region, and that use of this relationship, combined with the Doppler width of the broad emission line, enables an estimate of the mass of the black hole at the center of the active nucleus based on a single spectrum. An unresolved key issue is the choice of parameter used to characterize the line width, either FWHM or line dispersion σline (the square root of the second moment of the line profile). We argue here that use of FWHM introduces a bias, stretching the mass scale such that high masses are overestimated and low masses are underestimated. Here we investigate estimation of black hole masses in AGNs based on individual or "single-epoch" observations, with a particular emphasis in comparing mass estimates based on line dispersion and FWHM. We confirm the recent findings that, in addition to luminosity and line width, a third parameter is required to obtain accurate masses, and that parameter seems to be Eddington ratio. We present simplified empirical formulae for estimating black hole masses from the Hβ λ4861 and C iv λ1549 emission lines. While the AGN continuum luminosity at 5100 Å is usually used to predict the Hβ reverberation lag, we show that the luminosity of the Hβ broad component can be used instead without any loss of precision, thus eliminating the difficulty of accurately accounting for the host-galaxy contribution to the observed luminosity.
dc.relation.ispartofAstrophysical Journalen
dc.rightsCopyright © 2020. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of theCreative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.en
dc.subjectActive galactic nucleien
dc.subjectSupermassive black holesen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.titleThe Sloan Digital Sky Survey Reverberation Mapping Project : estimating masses of black holes in quasars with single-epoch spectroscopyen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews.St Andrews Centre for Exoplanet Scienceen
dc.description.statusPeer revieweden

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