Measurement of the supermassive black hole masses in two active galactic nuclei by the photometric reverberation mapping method
arXiv:2103.05801 · doi:10.1134/S1063773720110055
Abstract
We present the results of long-term photometric monitoring of two active galactic nuclei, 2MASX J08535955+7700543 (z 0.106) and VII Zw 244 (z 0.131), being investigated by the reverberation mapping method in medium-band filters. To estimate the size of the broad line region, we have analyzed the light curves with the JAVELIN code. The emission line widths have been measured using the spectroscopic data obtained at the 6-m BTA telescope of SAO RAS. We give our estimates of the supermassive black hole masses , , and , respectively
9 pages, 5 figures
References in corpus (8)
- Mean Spectral Energy Distributions and Bolometric Corrections for Luminous Quasars
- The Sloan Digital Sky Survey Reverberation Mapping Project: MgII Lag Results from Four Years of Monitoring
- Time-delay measurement of MgII broad line response for the highly-accreting quasar HE 0413-4031: Implications for the MgII-based radius-luminosity relation
- Dark matter in galaxies
- Mapper of Narrow Galaxy Lines (MaNGaL): new tunable filter imager for Caucasian telescopes
- SCORPIO-2 Guiding and Calibration System in the Prime Focus of the 6-m Telescope
- Stokes-polarimeter for 1-meter telescope
- Photometric reverberation mapping of AGNs at 0.1 < z < 0.8: I. Observational technique
Cited by in corpus (5)
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