Reverberation Mapping Results from MDM Observatory
Kelly D. Denney (OSU), B. M. Peterson (OSU), R. W. Pogge (OSU), M. C., Bentz (UC Irvine), C. M. Gaskell (UT Austin), T. Minezaki (U of Tokyo), C. A., Onken (Mount Stromlo Observatory), S. G. Sergeev (CrAO), M. Vestergaard (U of, Copenhagen)

TL;DR
This paper reports on a multi-month reverberation mapping campaign at MDM Observatory, measuring BLR radii and black hole masses for six objects, revealing diverse kinematic signatures in the BLR through velocity-resolved analysis.
Contribution
It provides new measurements of BLR sizes and black hole masses for six objects, with detailed velocity-resolved analysis of the H_beta response, highlighting diverse BLR kinematics.
Findings
Measured BLR radii and black hole masses for six objects
Identified diverse kinematic signatures in the BLR
Demonstrated the effectiveness of velocity-resolved analysis
Abstract
We present results from a multi-month reverberation mapping campaign undertaken primarily at MDM Observatory with supporting observations from around the world. We measure broad line region (BLR) radii and black hole masses for six objects. A velocity-resolved analysis of the H_beta response shows the presence of diverse kinematic signatures in the BLR.
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