9 research outputs found
BASS. XXX. Distribution functions of DR2 Eddington ratios, black hole masses, and X-ray luminosities
Galaxie
BASS XXXVII: the role of radiative feedback in the growth and obscuration properties of nearby supermassive black holes
Galaxie
Probing the structure and evolution of BASS active galactic nuclei through Eddington ratios
Galaxie
BASS. XXX. Distribution functions of DR2 Eddington ratios, black hole masses, and X-ray luminosities
BASS XXXVII: the role of radiative feedback in the growth and obscuration properties of nearby supermassive black holes
Probing the structure and evolution of BASS active galactic nuclei through Eddington ratios
Galaxie
BASS. XXV. DR2 broad-line-based black hole mass estimates and biases from obscuration
Galaxie
BASS. XXV. DR2 broad-line-based black hole mass estimates and biases from obscuration
We present measurements of broad emission lines and virial estimates of
supermassive black hole masses () for a large sample of ultra-hard
X-ray selected active galactic nuclei (AGNs) as part of the second data release
of the BAT AGN Spectroscopic Survey (BASS/DR2). Our catalog includes
estimates for a total 689 AGNs, determined from the H, H,
, and/or broad emission lines. The core
sample includes a total of 512 AGNs drawn from the 70-month Swift/BAT all-sky
catalog. We also provide measurements for 177 additional AGNs that are drawn
from deeper Swift/BAT survey data. We study the links between
estimates and line-of-sight obscuration measured from X-ray spectral analysis.
We find that broad H emission lines in obscured AGNs () are on average a factor of
weaker, relative to ultra-hard X-ray emission, and about \%
narrower than in unobscured sources (i.e., ). This indicates that the innermost part of the broad-line region is
preferentially absorbed. Consequently, current single-epoch
prescriptions result in severely underestimated (1 dex) masses for Type 1.9
sources (AGNs with broad H but no broad H) and/or sources with
. We provide simple multiplicative
corrections for the observed luminosity and width of the broad H
component ( and FWHM[bH]) in such sources to
account for this effect, and to (partially) remedy estimates for Type
1.9 objects. As key ingredient of BASS/DR2, our work provides the community
with the data needed to further study powerful AGNs in the low-redshift
Universe.Comment: published in ApJ