The Astrophysical Journal (Jan 2023)

The Seoul National University AGN Monitoring Project. IV. Hα Reverberation Mapping of Six AGNs and the Hα Size–Luminosity Relation

  • Hojin Cho,
  • Jong-Hak Woo,
  • Shu Wang,
  • Donghoon Son,
  • Jaejin Shin,
  • Suvendu Rakshit,
  • Aaron J. Barth,
  • Vardha N. Bennert,
  • Elena Gallo,
  • Edmund Hodges-Kluck,
  • Tommaso Treu,
  • Hyun-Jin Bae,
  • Wanjin Cho,
  • Adi Foord,
  • Jaehyuk Geum,
  • Yashashree Jadhav,
  • Yiseul Jeon,
  • Kyle M. Kabasares,
  • Daeun Kang,
  • Wonseok Kang,
  • Changseok Kim,
  • Donghwa Kim,
  • Minjin Kim,
  • Taewoo Kim,
  • Huynh Anh N. Le,
  • Matthew A. Malkan,
  • Amit Kumar Mandal,
  • Daeseong Park,
  • Songyoun Park,
  • Hyun-il Sung,
  • Vivian U,
  • Peter R. Williams

DOI
https://doi.org/10.3847/1538-4357/ace1e5
Journal volume & issue
Vol. 953, no. 2
p. 142

Abstract

Read online

The broad-line region (BLR) size–luminosity relation has paramount importance for estimating the mass of black holes in active galactic nuclei (AGNs). Traditionally, the size of the H β BLR is often estimated from the optical continuum luminosity at 5100 Å, while the size of the H α BLR and its correlation with the luminosity is much less constrained. As a part of the Seoul National University AGN Monitoring Project, which provides 6 yr photometric and spectroscopic monitoring data, we present our measurements of the H α lags of high-luminosity AGNs. Combined with the measurements for 42 AGNs from the literature, we derive the size–luminosity relations of the H α BLR against the broad H α and 5100 Å continuum luminosities. We find the slope of the relations to be 0.61 ± 0.04 and 0.59 ± 0.04, respectively, which are consistent with the H β size–luminosity relation. Moreover, we find a linear relation between the 5100 Å continuum luminosity and the broad H α luminosity across 7 orders of magnitude. Using these results, we propose a new virial mass estimator based on the H α broad emission line, finding that the previous mass estimates based on scaling relations in the literature are overestimated by up to 0.7 dex at masses lower than 10 ^7 M _⊙ .

Keywords