TY - JOUR
T1 - The sloan digital sky survey reverberation mapping project
T2 - Estimating masses of black holes in Quasars with single-epoch spectroscopy
AU - Bontà, Elena Dalla
AU - Peterson, Bradley M.
AU - Bentz, Misty C.
AU - Brandt, W. N.
AU - Ciroi, S.
AU - De Rosa, Gisella
AU - Alvarez, Gloria Fonseca
AU - Grier, Catherine J.
AU - Hall, P. B.
AU - Santisteban, Juan V.Hernández
AU - Ho, Luis C.
AU - Homayouni, Y.
AU - Horne, Keith
AU - Kochanek, C. S.
AU - Li, Jennifer I.Hsiu
AU - Morelli, L.
AU - Pizzella, A.
AU - Pogge, R. W.
AU - Schneider, D. P.
AU - Shen, Yue
AU - Trump, J. R.
AU - Vestergaard, Marianne
N1 - Publisher Copyright:
© 2020 The Author(s).
PY - 2020/11/10
Y1 - 2020/11/10
N2 - 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 A 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.
AB - 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 A 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.
UR - http://www.scopus.com/inward/record.url?scp=85095509541&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85095509541&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/abbc1c
DO - 10.3847/1538-4357/abbc1c
M3 - Article
AN - SCOPUS:85095509541
SN - 0004-637X
VL - 903
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 112
ER -