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Virial black hole mass ($M_{BH}$) determination directly involves knowing the broad line region (BLR) clouds velocity distribution, their distance from the central supermassive black hole ($R_{BLR}$) and the virial factor ($f$). Understanding whether biases arise in $M_{BH}$ estimation with increasing obscuration is possible only by studying a large (N$>$100) statistical sample of obscuration unbiased (hard) X-ray selected active galactic nuclei (AGN) in the rest-frame near-infrared (0.8-2.5$\mu$m) since it penetrates deeper into the BLR than the optical. We present a detailed analysis of 65 local BAT-selected Seyfert galaxies observed with Magellan/FIRE. Adding these to the near-infrared BAT AGN spectroscopic survey (BASS) database, we study a total of 314 unique near-infrared spectra. While the FWHMs of H$\alpha$ and near-infrared broad lines (He\textsc{i}, Pa$\beta$, Pa$\alpha$) remain unbiased to either BLR extinction or X-ray obscuration, the H$\alpha$ broad line luminosity is suppressed when $N_H\gtrsim10^{21}$ cm$^{-2}$, systematically underestimating $M_{BH}$ by $0.23-0.46$ dex. Near-infrared line luminosities should be preferred to H$\alpha$ until $N_H<10^{22}$ cm$^{-2}$, while at higher obscuration a less biased $R_{BLR}$ proxy should be adopted. We estimate $f$ for Seyfert 1 and 2 using two obscuration-unbiased $M_{BH}$ measurements, i.e. the stellar velocity dispersion and a BH mass prescription based on near-infrared and X-ray, and find that the virial factors do not depend on redshift or obscuration, but for some broad lines show a mild anti-correlation with $M_{BH}$. Our results show the critical impact obscuration can have on BLR characterization and the importance of the near-infrared and X-rays for a less biased view of the BLR., Comment: 28 pages (excluding appendices), 14 figures, pre-proof version accepted for publication on ApJ (to appear on the BASS DR2 ApJ Special Issue)

Virial black hole mass ($M_{BH}$) determination directly involves knowing the broad line region (BLR) clouds velocity distribution, their distance from the central supermassive black hole ($R_{BLR}$) and the virial factor ($f$). Understanding whether biases arise in $M_{BH}$ estimation with increasing obscuration is possible only by studying a large (N$>$100) statistical sample of obscuration unbiased (hard) X-ray selected active galactic nuclei (AGN) in the rest-frame near-infrared (0.8-2.5$\mu$m) since it penetrates deeper into the BLR than the optical. We present a detailed analysis of 65 local BAT-selected Seyfert galaxies observed with Magellan/FIRE. Adding these to the near-infrared BAT AGN spectroscopic survey (BASS) database, we study a total of 314 unique near-infrared spectra. While the FWHMs of H$\alpha$ and near-infrared broad lines (He\textsc{i}, Pa$\beta$, Pa$\alpha$) remain unbiased to either BLR extinction or X-ray obscuration, the H$\alpha$ broad line luminosity is suppressed when $N_H\gtrsim10^{21}$ cm$^{-2}$, systematically underestimating $M_{BH}$ by $0.23-0.46$ dex. Near-infrared line luminosities should be preferred to H$\alpha$ until $N_H<10^{22}$ cm$^{-2}$, while at higher obscuration a less biased $R_{BLR}$ proxy should be adopted. We estimate $f$ for Seyfert 1 and 2 using two obscuration-unbiased $M_{BH}$ measurements, i.e. the stellar velocity dispersion and a BH mass prescription based on near-infrared and X-ray, and find that the virial factors do not depend on redshift or obscuration, but for some broad lines show a mild anti-correlation with $M_{BH}$. Our results show the critical impact obscuration can have on BLR characterization and the importance of the near-infrared and X-rays for a less biased view of the BLR., Comment: 28 pages (excluding appendices), 14 figures, pre-proof version accepted for publication on ApJ (to appear on the BASS DR2 ApJ Special Issue)