The Seoul National University AGN monitoring project. II. BLR size and black hole mass of two AGNs
Suvendu Rakshit, Jong-Hak Woo, Elena Gallo, Edmund Hodges-Kluck, Jaejin Shin, Yiseul Jeon, Hyun-Jin Bae, Vivienne Baldassare, Hojin Cho, Wanjin Cho, Adi Foord, … 展开作者
Suvendu Rakshit, Jong-Hak Woo, Elena Gallo, Edmund Hodges-Kluck, Jaejin Shin, Yiseul Jeon, Hyun-Jin Bae, Vivienne Baldassare, Hojin Cho, Wanjin Cho, Adi Foord, Daeun Kang, Wonseok Kang, Marios Karouzos, Minjin Kim, Taewoo Kim, Huynh Anh N. Le, Daeseong Park, Songyoun Park, Donghoon Son, Hyun-il Sung, Vardha N. Bennert, Matthew A. Malkan
活动星系核（AGN）的宽线区（BLR）的大小和单色连续发光度在5100度之间的相关性，允许黑洞质量估计的基础上单历元光谱。然而，相关性的有效性还有待明确的高光度活动星系核测试。我们提出了第一个混响映射结果的首尔国立大学活动星系核监测计划（SAMP），这是专为专注于发光活动星系核探测高端的大小-光度关系。本文报道了两个活动星系核（2 MASS J10261389+5237510和SDSS J161911.24+501109.2）的光变曲线测量结果，测量周期为$\sim$ 1000天，平均周期为$\sim$ 10天和$\sim$ 20天，分别用于光度测量和光谱测量。基于互相关分析和H $β$线宽测量，我们确定了2 MASS J1026和SDSS J1619的H $β$滞后为$41.8^{+4.9}_{-6.0}$和$52.6^{+17.6}_{-14.7}$天，黑洞质量分别为$3.65^{+0.49}_{-0.57} \times 10^7 M_{\odot}$和$23.02^{+7.81}_{-6.56} \times 10^7 M_{\odot}$.
英文摘要：
Active galactic nuclei (AGNs) show a correlation between the size of the broad line region (BLR) and the monochromatic continuum luminosity at 5100 Å, 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$20 days, respectively for photometry and spectroscopy monitoring. Based on a cross-correlation analysis and H$β$ line width measurements, we determine the H$β$ 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.
The Seoul National University AGN Monitoring Project III: H$β$ lag measurements of 32 luminous AGNs and the high-luminosity end of the size--luminosity relation
Can BLR line profile shape improve single-epoch black hole mass estimates?
California Polytechnic State University（加州州立理工大学）；University of California, Los Angeles（加州大学洛杉矶分校）；Seoul National University（首尔大学）；Georgia State University（佐治亚州立大学）；The University of Auckland（奥克兰大学）；University of California, Irvine（加州大学尔湾分校）；Caltech/IPAC（加州理工学院/IPAC）
Diverse Origins of Broad H$α$ Lines in Heavily Obscured AGNs Revealed by Multi-epoch Spectroscopy
Academia Sinica Institute of Astronomy and Astrophysics（中央研究院天文及天文物理研究所）；The University of Tokyo（东京大学）；National Astronomical Observatory of Japan（日本国立天文台）
Understanding the Broad-line Region of Active Galactic Nuclei with Photoionization. II. Slim disks, Self-shadowing, and BLR sizes
University of Illinois at Urbana-Champaign（伊利诺伊大学厄巴纳-香槟分校）；National Center for Supercomputing Applications, University of Illinois at Urbana-Champaign（伊利诺伊大学厄巴纳-香槟分校超级计算应用国家中心）；Durham University（杜伦大学）；University of Leicester（莱斯特大学）；IFPU - Institute for Fundamental Physics of the Universe（宇宙基础物理研究所）；SISSA - International School for Advanced Studies（高等研究院）；INAF - Osservatorio Astronomico di Trieste（的里雅斯特天文台）
The 2MIG isolated AGNs -- 4. Linking hot-dust reverberation to spectroscopically predicted BLR scales in IC~5287 and Mrk~845
Main Astronomical Observatory of the NAS of Ukraine（乌克兰国家科学院主天文台）；International Centre for Astronomical, Medical and Ecological Research (ICAMER)（国际天体医学与生态研究中心）；Instituto de Astrofísica de Canarias（加那利群岛天体物理研究所）；Departamento de Astrofísica, Universidad de la Laguna（拉古纳大学天体物理学系）
Dynamical Modeling of the Broad-Line Region with High-Mass Active Galactic Nuclei and Constraints on the Virial Factor
Seoul National University（首尔大学）；California Polytechnic State University（加州州立理工大学）；University of California, Los Angeles（加州大学洛杉矶分校）；University of Michigan（密歇根大学）
The First Detection of Forbidden Emission Lines at the Outskirts of the AGN Broad Line Region?
Universidade Federal de Santa Maria（圣玛丽亚联邦大学）；Universidade de São Paulo（圣保罗大学）；Universidade Federal da Fronteira Sul（南部边境联邦大学）；Universidade do Vale do Paraíba（帕拉伊巴河谷大学）
Black Holes in the Shadow: The Missing High-Ionization Lines in the Earliest JWST AGNs
Università degli Studi di Milano-Bicocca（米兰比可卡大学）；Stockholm University（斯德哥尔摩大学）；University of Cambridge（剑桥大学）；University College London（伦敦大学学院）；University of California Santa Cruz（加州大学圣克鲁兹分校）
Detection of unexpected leading delays in broad Hβ line reverberations in the quasar PHL 1092
Institute of High Energy Physics, Chinese Academy of Sciences（中国科学院高能物理研究所）；University of Chinese Academy of Sciences（中国科学院大学）；National Astronomical Observatories of China, Chinese Academy of Sciences（中国科学院国家天文台）；Technology and Engineering Center for Space Utilization, Chinese Academy of Sciences（中国科学院空间应用工程与技术中心）；Nanjing University（南京大学）；University of Wyoming（怀俄明大学）；Yunnan Observatory, Chinese Academy of Sciences（中国科学院云南天文台）；Anyang Normal University（安阳师范学院）；Centro Astronomico Hispano Alemán（德西天体观测中心）；Instituto de Astrofisica de Andalucía（安达卢西亚天体物理学研究所）
The Most Luminous H$β$ Reverberation Mapping of E1821+643 Indicates the Lower Boundary of the Radius-Luminosity Relation
Yunnan Observatories, Chinese Academy of Sciences（中国科学院云南天文台）；Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences（中国科学院天体结构与演化重点实验室）；Center for Astronomical Mega-Science, Chinese Academy of Sciences（中国科学院天文大科学研究中心）；Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences（中国科学院射电天文与技术重点实验室）；Institute for Astronomy, School of Physics, Zhejiang University（浙江大学物理学院天体物理研究所）
Anisotropic Radiation in Super-Eddington Active Galactic Nuclei: The Responsivity of Broad-Line Regions to Continuum Variability
State Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences（高能物理研究所粒子天体物理国家重点实验室）；National Astronomical Observatories, Chinese Academy of Sciences（中国科学院国家天文台）；School of Astronomy and Space Science, University of Chinese Academy of Sciences（中国科学院大学天文与空间科学学院）
