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Monitoring AGNs with Hβ Asymmetry. IV. First Reverberation Mapping Results of 14 Active Galactic Nuclei

文献类型：期刊论文

作者Zastrocky, T. E.21; Brotherton, Michael S.21; Du, Pu20; McLane, Jacob N.21; Olson, Kianna A.21; Dale, D. A.21; Kobulnicky, H. A.21; Maithil, Jaya19; Nguyen, My L.21; Chick, William T.21
刊名ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
出版日期2024-06-01
卷号272期号:2
ISSN号0067-0049
DOI10.3847/1538-4365/ad3bad
产权排序第18完成单位
文献子类Article
英文摘要We report first-time reverberation-mapping results for 14 active galactic nuclei (AGNs) from the ongoing Monitoring AGNs with H beta Asymmetry campaign (MAHA). These results utilize optical spectra obtained with the Long Slit Spectrograph on the Wyoming Infrared 2.3 m Telescope between 2017 November and 2023 May. MAHA combines long-duration monitoring with high cadence. We report results from multiple observing seasons for nine of the 14 objects. These results include H beta time lags, supermassive black hole masses, and velocity-resolved time lags. The velocity-resolved lags allow us to investigate the kinematics of the broad-line region.
学科主题天文学 ; 星系与宇宙学
URL标识查看原文
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
WOS关键词BROAD-LINE REGION ; SUPERMASSIVE BLACK-HOLES ; HIGH ACCRETION RATES ; FE II REVERBERATION ; SEYFERT-GALAXIES ; M-BH-SIGMA(ASTERISK) RELATION ; OPTICAL CONTINUUM ; SPACE TELESCOPE ; CENTRAL MASSES ; NGC 5548
资助项目NSF divided by National Science Foundation Graduate Research Fellowship Program (GRFP)https://doi.org/10.13039/100023581[11721303]; NSF divided by National Science Foundation Graduate Research Fellowship Program (GRFP)https://doi.org/10.13039/100023581[11991052]; NSF divided by National Science Foundation Graduate Research Fellowship Program (GRFP)https://doi.org/10.13039/100023581[12011540375]; NSF divided by National Science Foundation Graduate Research Fellowship Program (GRFP)https://doi.org/10.13039/100023581[12233001]; National Science Foundation of China[2021YFA1600404]; National Key R&D Program of China[CMS-CSST-2021-A04]; National Key R&D Program of China[CMS-CSST-2021-A06]; China Manned Space Project[AST 1852289]; National Science Foundation under REU[NSFC-12022301]; National Science Foundation under REU[-11873048]; NSFC[1005444I]; NSF[759194]; National Aeronautics and Space Administration - European Research Council (ERC) under the European Union; Zwicky Transient Facility project[AST-1440341]; National Science Foundation; Weizmann Institute for Science; Oskar Klein Center at Stockholm University; University of Washington, Deutsches Elektronen-Synchrotron and Humboldt University, Los Alamos National Laboratories; TANGO Consortium of Taiwan; University of Wisconsin at Milwaukee; Lawrence Berkeley National Laboratories
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001225573700001
出版者IOP Publishing Ltd
资助机构NSF divided by National Science Foundation Graduate Research Fellowship Program (GRFP)https://doi.org/10.13039/100023581[11721303, 11991052, 12011540375, 12233001] ; National Science Foundation of China[2021YFA1600404] ; National Key R&D Program of China[CMS-CSST-2021-A04, CMS-CSST-2021-A06] ; China Manned Space Project[AST 1852289] ; National Science Foundation under REU[NSFC-12022301, -11873048] ; NSFC[1005444I] ; NSF[759194] ; National Aeronautics and Space Administration - European Research Council (ERC) under the European Union ; Zwicky Transient Facility project[AST-1440341] ; National Science Foundation ; Weizmann Institute for Science ; Oskar Klein Center at Stockholm University ; University of Washington, Deutsches Elektronen-Synchrotron and Humboldt University, Los Alamos National Laboratories ; TANGO Consortium of Taiwan ; University of Wisconsin at Milwaukee ; Lawrence Berkeley National Laboratories
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/27203]  
专题云南天文台_丽江天文观测站（南方基地）
作者单位1.Department of Physics, Grinnell College, Grinnell, IA 50112, USA;
2.National Astronomical Observatories of China, Chinese Academy of Sciences, 20A Datun Road, Beijing 100020, People's Republic of China
3.Department of Astronomy, School of Physics, Peking University, Beijing 100871, People's Republic of China;
4.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People's Republic of China;
5.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, People's Republic of China;
6.School of Astronomy and Space Science, University of Chinese Academy of Sciences, 19A Yuquan Road, Beijing 100049, People's Republic of China;
7.Department of Physics, Illinois Institute of Technology, Chicago, IL 60616, USA;
8.Department of Physics and Astronomy, Cal Poly Humboldt, Arcata, CA 95521, USA;
9.Department of Astronomy, Whitman College, Walla Walla, WA 99362, USA;
10.Department of Physics, Oklahoma Baptist University, Shawnee, OK 74804, USA;
推荐引用方式
GB/T 7714		 Zastrocky, T. E.,Brotherton, Michael S.,Du, Pu,et al. Monitoring AGNs with Hβ Asymmetry. IV. First Reverberation Mapping Results of 14 Active Galactic Nuclei[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2024,272(2).
APA Zastrocky, T. E..,Brotherton, Michael S..,Du, Pu.,McLane, Jacob N..,Olson, Kianna A..,...&Wang, Jian-Min.(2024).Monitoring AGNs with Hβ Asymmetry. IV. First Reverberation Mapping Results of 14 Active Galactic Nuclei.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,272(2).
MLA Zastrocky, T. E.,et al."Monitoring AGNs with Hβ Asymmetry. IV. First Reverberation Mapping Results of 14 Active Galactic Nuclei".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 272.2(2024).

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来源：云南天文台

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