%0 Generic %1 mejiarestrepo2022broadline %A Mejıa-Restrepo, Julian E. %A Trakhtenbrot, Benny %A Koss, Michael J. %A Oh, Kyuseok %A Brok, Jakob den %A Stern, Daniel %A Powell, Meredith C. %A Ricci, Federica %A Caglar, Turgay %A Ricci, Claudio %A Bauer, Franz E. %A Treister, Ezequiel %A Harrison, Fiona A. %A Urry, C. M. %A Ananna, Tonima Tasnim %A Asmus, Daniel %A Assef, Roberto J. %A Bar, Rudolf E. %A Bessiere, Patricia S. %A Burtscher, Leonard %A Ichikawa, Kohei %A Kakkad, Darshan %A Kamraj, Nikita %A Mushotzky, Richard %A Privon, George C. %A Rojas, Alejandra F. %A Sani, Eleonora %A Schawinski, Kevin %A Veilleux, Sylvain %D 2022 %K library %T BASS XXV: DR2 Broad-line Based Black Hole Mass Estimates and Biases from Obscuration %U http://arxiv.org/abs/2204.05321 %X We present measurements of broad emission lines and virial estimates of supermassive black hole masses ($M_BH$) 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 $M_BH$ estimates for a total 689 AGNs, determined from the H$\alpha$, H$\beta$, $MgIIłambda2798$, and/or $CIVłambda1549$ 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 $M_BH$ estimates and line-of-sight obscuration measured from X-ray spectral analysis. We find that broad H$\alpha$ emission lines in obscured AGNs ($(N_\rm H/cm^-2)> 22.0$) are on average a factor of $8.0_-2.4^+4.1$ weaker, relative to ultra-hard X-ray emission, and about $35_-12^~+7$\% narrower than in unobscured sources (i.e., $(N_H/cm^-2) < 21.5$). This indicates that the innermost part of the broad-line region is preferentially absorbed. Consequently, current single-epoch $M_BH$ prescriptions result in severely underestimated ($>$1 dex) masses for Type 1.9 sources (AGNs with broad H$\alpha$ but no broad H$\beta$) and/or sources with $(N_H/cm^-2) > 22.0$. We provide simple multiplicative corrections for the observed luminosity and width of the broad H$\alpha$ component ($LbH\alpha$ and FWHMbH$\alpha$) in such sources to account for this effect, and to (partially) remedy $M_BH$ 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.

@misc{mejiarestrepo2022broadline, abstract = {We present measurements of broad emission lines and virial estimates of supermassive black hole masses ($M_{BH}$) 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 $M_{BH}$ estimates for a total 689 AGNs, determined from the H$\alpha$, H$\beta$, $MgII\lambda2798$, and/or $CIV\lambda1549$ 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 $M_{BH}$ estimates and line-of-sight obscuration measured from X-ray spectral analysis. We find that broad H$\alpha$ emission lines in obscured AGNs ($\log (N_{\rm H}/{\rm cm}^{-2})> 22.0$) are on average a factor of $8.0_{-2.4}^{+4.1}$ weaker, relative to ultra-hard X-ray emission, and about $35_{-12}^{~+7}$\% narrower than in unobscured sources (i.e., $\log (N_{\rm H}/{\rm cm}^{-2}) < 21.5$). This indicates that the innermost part of the broad-line region is preferentially absorbed. Consequently, current single-epoch $M_{BH}$ prescriptions result in severely underestimated ($>$1 dex) masses for Type 1.9 sources (AGNs with broad H$\alpha$ but no broad H$\beta$) and/or sources with $\log (N_{\rm H}/{\rm cm}^{-2}) > 22.0$. We provide simple multiplicative corrections for the observed luminosity and width of the broad H$\alpha$ component ($L[{\rm b}{\rm H}\alpha]$ and FWHM[bH$\alpha$]) in such sources to account for this effect, and to (partially) remedy $M_{BH}$ 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.}, added-at = {2022-04-13T09:16:29.000+0200}, author = {Mejıa-Restrepo, Julian E. and Trakhtenbrot, Benny and Koss, Michael J. and Oh, Kyuseok and Brok, Jakob den and Stern, Daniel and Powell, Meredith C. and Ricci, Federica and Caglar, Turgay and Ricci, Claudio and Bauer, Franz E. and Treister, Ezequiel and Harrison, Fiona A. and Urry, C. M. and Ananna, Tonima Tasnim and Asmus, Daniel and Assef, Roberto J. and Bar, Rudolf E. and Bessiere, Patricia S. and Burtscher, Leonard and Ichikawa, Kohei and Kakkad, Darshan and Kamraj, Nikita and Mushotzky, Richard and Privon, George C. and Rojas, Alejandra F. and Sani, Eleonora and Schawinski, Kevin and Veilleux, Sylvain}, biburl = {https://www.bibsonomy.org/bibtex/21914721423e8ed842c9a1fe0567808c1/gpkulkarni}, description = {BASS XXV: DR2 Broad-line Based Black Hole Mass Estimates and Biases from Obscuration}, interhash = {7566f2edb3d7f20cff8701618aadf6d8}, intrahash = {1914721423e8ed842c9a1fe0567808c1}, keywords = {library}, note = {cite arxiv:2204.05321Comment: Accepted for publication in ApJS}, timestamp = {2022-04-13T09:16:29.000+0200}, title = {BASS XXV: DR2 Broad-line Based Black Hole Mass Estimates and Biases from Obscuration}, url = {http://arxiv.org/abs/2204.05321}, year = 2022 }