The Sloan Digital Sky Survey Reverberation Mapping Project: estimating masses of black holes in quasars with single-epoch spectroscopy

Elena Dalla Bontà, Bradley M. Peterson, Misty C. Bentz, W. N. Brandt, Stefano Ciroi, Gisella De Rosa, Gloria Fonseca Alvarez, Catherine J. Grier, P. B. Hall, Juan V. Hernandez Santisteban, Luis C. Ho, Y. Homayouni, Keith Horne, C. S. Kochanek, Jennifer I-Hsiu Li, Lorenzo Morelli, Alessandro Pizzella, R. W. Pogge, D. P. Schneider, Yue ShenJ. R. Trump, Marianne Vestergaard

Research output: Contribution to journalArticlepeer-review

26 Citations (Scopus)

Abstract

It 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.
Original languageEnglish
Article number112
Number of pages28
JournalAstrophysical Journal
Volume903
Issue number2
Early online date9 Nov 2020
DOIs
Publication statusPublished - 10 Nov 2020

Keywords

  • Active galactic nuclei
  • Quasars
  • Supermassive black holes

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