BASS XXV: DR2 Broad-line Based Black Hole Mass Estimates and Biases from Obscuration
arXiv:2204.05321 · doi:10.3847/1538-4365/ac6602
Abstract
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.
published in ApJS
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