中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A New Approach to Constraining Properties of Active Galactic Nucleus Host Galaxies by Combining Image and Spectral Energy Distribution Decomposition: Testing upon the MBH-M☆ Relation

文献类型:期刊论文

作者Yu, Haoran4,5; Fan, Lulu3,4,5; Han YK(韩云坤)1,2,6,8; Sun, Weibin4,5; Zhang, Yihang4,5; Ding, Xuheng7; Xue, Yongquan4,5
刊名ASTROPHYSICAL JOURNAL
出版日期2025-01-10
卷号978期号:2
ISSN号0004-637X
DOI10.3847/1538-4357/ad9aa3
产权排序第4完成单位
文献子类Article
英文摘要The outshining light from active galactic nuclei (AGNs) poses significant challenges in studying the properties of AGN host galaxies. To address this issue, we propose a novel approach that combines image decomposition and spectral energy distribution (SED) decomposition to constrain the properties of AGN host galaxies. Image decomposition allows us to disentangle optical flux into AGN and stellar components, thereby providing additional constraints on the SED models to derive a more refined stellar mass. To test the viability of this approach, we obtained a sample of 24 X-ray-selected type I AGNs with redshifts ranging from 0.73 to 2.47. We estimated the stellar masses for our sample and found that our results are generally consistent with earlier estimates based on different methods. Through examining the posterior distribution of stellar masses, we find that our method could derive better-constrained results compared to previous SED decomposition methods. With the derived stellar masses, we further studied the MBH-M star relation of our sample, finding a higher intrinsic scatter in the correlation for our entire sample compared to the local quiescent correlation, which could be caused by a few black hole monsters in our sample. We propose that, based on our method, future works could extend to larger samples of high-redshift AGN host galaxies, thereby enhancing our understanding of their properties.
学科主题天文学 ; 恒星与银河系
URL标识查看原文
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
WOS关键词SUPERMASSIVE BLACK-HOLES ; REVERBERATION MAPPING PROJECT ; TOTAL STELLAR MASS ; BROAD-LINE AGNS ; SCALING RELATIONS ; COSMIC EVOLUTION ; BULGE MASS ; LEGACY SURVEY ; GROWTH ; SPACE
资助项目National Key Research and Development Program of China[2023YFA1608100]; National Natural Science Foundation of China (NSFC)[12173037]; National Natural Science Foundation of China (NSFC)[12233008]; National Natural Science Foundation of China (NSFC)[11773063]; National Natural Science Foundation of China (NSFC)[12288102]; National Natural Science Foundation of China (NSFC)[12025303]; CAS Project for Young Scientists in Basic Research[YSBR-092]; China Manned Space Project[CMS-CSST-2021-A02]; China Manned Space Project[CMS-CSST-2021-A04]; China Manned Space Project[CMS-CSST-2021-A06]; Fundamental Research Funds for Central Universities[WK3440000006]; Cyrus Chun Ying Tang Foundations; National Key R&D Program of China[2021YFA1600401]; National Key R&D Program of China[2021YFA1600400]; Light of West China Program of the Chinese Academy of Sciences; Yunnan Ten Thousand Talents Plan Young & Elite Talents Project; Natural Science Foundation of Yunnan Province[202201BC070003]; International Centre of Supernovae, Yunnan Key Laboratory[202302AN360001]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001394223700001
出版者IOP Publishing Ltd
资助机构National Key Research and Development Program of China[2023YFA1608100] ; National Natural Science Foundation of China (NSFC)[12173037, 12233008, 11773063, 12288102, 12025303] ; CAS Project for Young Scientists in Basic Research[YSBR-092] ; China Manned Space Project[CMS-CSST-2021-A02, CMS-CSST-2021-A04, CMS-CSST-2021-A06] ; Fundamental Research Funds for Central Universities[WK3440000006] ; Cyrus Chun Ying Tang Foundations ; National Key R&D Program of China[2021YFA1600401, 2021YFA1600400] ; Light of West China Program of the Chinese Academy of Sciences ; Yunnan Ten Thousand Talents Plan Young & Elite Talents Project ; Natural Science Foundation of Yunnan Province[202201BC070003] ; International Centre of Supernovae, Yunnan Key Laboratory[202302AN360001]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/27984]  
专题云南天文台_大样本恒星演化研究组
云南天文台_中国科学院天体结构与演化重点实验室
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, People's Republic of China; hanyk@ynao.ac.cn;
2.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, People's Republic of China;
3.Deep Space Exploration Laboratory, Hefei 230088, People's Republic of China;
4.School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, People's Republic of China;
5.CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei 230026, People's Republic of China; llfan@ustc.edu.cn;
6.International Centre of Supernovae, Yunnan Key Laboratory, Kunming 650216, People's Republic of China;
7.School of Physics and Technology, Wuhan University, Wuhan 430072, People's Republic of China
8.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, People's Republic of China;
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Yu, Haoran,Fan, Lulu,Han YK,et al. A New Approach to Constraining Properties of Active Galactic Nucleus Host Galaxies by Combining Image and Spectral Energy Distribution Decomposition: Testing upon the MBH-M☆ Relation[J]. ASTROPHYSICAL JOURNAL,2025,978(2).
APA Yu, Haoran.,Fan, Lulu.,韩云坤.,Sun, Weibin.,Zhang, Yihang.,...&Xue, Yongquan.(2025).A New Approach to Constraining Properties of Active Galactic Nucleus Host Galaxies by Combining Image and Spectral Energy Distribution Decomposition: Testing upon the MBH-M☆ Relation.ASTROPHYSICAL JOURNAL,978(2).
MLA Yu, Haoran,et al."A New Approach to Constraining Properties of Active Galactic Nucleus Host Galaxies by Combining Image and Spectral Energy Distribution Decomposition: Testing upon the MBH-M☆ Relation".ASTROPHYSICAL JOURNAL 978.2(2025).

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来源:云南天文台

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