Active galactic nuclei (AGNs) show a correlation between the size of the broad line region (BLR) and the monochromatic continuum luminosity at 5100 \AA, allowing black hole mass estimation based on single-epoch spectra. However, the validity of the correlation is yet to be clearly tested for high-luminosity AGNs. We present the first reverberation-mapping results of the Seoul National University AGN monitoring program (SAMP), which is designed to focus on luminous AGNs for probing the high end of the size-luminosity relation. We report time lag measurements of two AGNs, namely, 2MASS J10261389+5237510 and SDSS J161911.24+501109.2, using the light curves obtained over a $\sim$1000 day period with an average cadence of $\sim$10 and $\sim$20 days, respectively for photometry and spectroscopy monitoring. Based on a cross-correlation analysis and H$\beta$ line width measurements, we determine the H$\beta$ lag as $41.8^{ +4.9}_{ -6.0}$ and $52.6^{ +17.6}_{ -14.7}$ days in the observed-frame, and black hole mass as $3.65^{ +0.49}_{ -0.57} \times 10^7 M_{ \odot}$ and $23.02^{ +7.81}_{ -6.56} \times 10^7 M_{ \odot}$, respectively for 2MASS J1026 and SDSS J1619.
Categories: astro-ph.GA