Spectroastrometry and Reverberation Mapping of Active Galactic Nuclei. I. The Hβ Broad-line Region Structure and Black Hole Masses of Five Quasars
Ho, Luis C.; Du, Pu; Hu, Chen; Wang, Jian-Min; Li, Yan-Rong; Aceituno, Jesús; Bai, Jin-Ming; Chen, Yong-Jie; Liu, Jun-Rong; Yang, Sen; Yao, Zhu-Heng; Zhai, Shuo; Xiao, Ming; Petrov, Romain G.; Fang, Feng-Na; Bai, Hua-Rui; Fu, Yi-Xin; Wang, Yi-Lin; Songsheng, Yu-Yang; Winkler, Hartmut; Peng, Yue-Chang
China, South Africa, France, Spain
Abstract
We conduct a reverberation mapping (RM) campaign to spectroscopically monitor a sample of selected bright active galactic nuclei with large anticipated broad-line region (BLR) sizes adequate for spectroastrometric (SA) observations by the GRAVITY instrument on the Very Large Telescope Interferometer. We report the first results for five objects, IC 4329A, Mrk 335, Mrk 509, Mrk 1239, and PDS 456, among which Mrk 1239 and PDS 456 are for the first time spectroscopically monitored. We obtain multiyear monitoring data and perform multicomponent spectral decomposition to extract the broad Hβ profiles. We detect significant time lags between the Hβ and continuum variations, generally obeying the previously established BLR size–luminosity relation. Velocity-resolved Hβ time lags illustrate diverse, possibly evolving, BLR kinematics. We further measure the Hβ line widths from mean and rms spectra and the resulting virial products show good consistency among different observing seasons. Adopting a unity virial factor and the FWHM of the broad Hβ line from the mean spectra as a measure of velocity, the obtained black hole masses averaged over seasons are