PMO OpenIR  > 暗物质和空间天文实验室
AGN host galaxies at redshift z approximate to 0.7: peculiar or not?
Boehm, A.1,2; Wisotzki, L.2; Bell, E. F.3; Jahnke, K.4; Wolf, C.5; Bacon, D.6; Barden, M.1; Gray, M. E.7; Hoeppe, G.8; Jogee, S.9; McIntosh, D. H.10; Peng, C. Y.11; Robaina, A. R.4,12; Balogh, M.13; Barazza, F. D.14; Caldwell, J. A. R.15; Heymans, C.16; Haeussler, B.7; van Kampen, E.17; Lane, K.7; Meisenheimer, K.4; Sanchez, S. F.18; Taylor, A. N.16; Zheng, X.19
2013
Source PublicationASTRONOMY & ASTROPHYSICS
ISSN0004-6361
Volume549Pages:A46-A46
Corresponding AuthorBohm, A (reprint author), Univ Innsbruck, Inst Astro & Particle Phys, Tech Str 25-8, A-6020 Innsbruck, Austria. Email: Asmus.Boehm@uibk.ac.at
AbstractAims. We perform a quantitative morphological comparison between the hosts of active galactic nuclei (AGN) and quiescent galaxies at intermediate redshifts (z approximate to 0.7). The imaging data are taken from the large HST/ACS mosaics of the GEMS and STAGES surveys. Our main aim is to test whether nuclear activity at this cosmic epoch is triggered by major mergers.
KeywordGalaxies: Active Galaxies: Interactions Galaxies: Evolution
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1051/0004-6361/201015444
WOS KeywordACTIVE GALACTIC NUCLEUS ; DIGITAL-SKY-SURVEY ; BLACK-HOLE GROWTH ; DEEP FIELD-SOUTH ; LUMINOSITY FUNCTION ; ELLIPTIC GALAXIES ; COMBO-17 SURVEY ; SMALL SCALES ; GEMS SURVEY ; EVOLUTION
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000313745000046
Citation statistics
Cited Times:32[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/9761
Collection暗物质和空间天文实验室
Affiliation1.Univ Innsbruck, Inst Astro & Particle Phys, A-6020 Innsbruck, Austria
2.Astrophys Inst Potsdam, D-14482 Potsdam, Germany
3.Univ Michigan, Dept Astron, Ann Arbor, MI 48105 USA
4.Max Planck Inst Astron, D-69117 Heidelberg, Germany
5.Univ Oxford, Dept Phys, Oxford OX1 3RH, England
6.Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 2EG, Hants, England
7.Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England
8.Univ Waterloo, Dept Anthropol, Waterloo, ON N2L 3G1, Canada
9.Univ Texas Austin, Dept Astron, Austin, TX 78712 USA
10.Univ Missouri Kansas City, Dept Phys, Kansas City, MO 64110 USA
11.Giant Magellan Telescope Org, Pasadena, CA 91101 USA
12.Univ Barcelona, Inst Ciencies Cosmos, E-08028 Barcelona, Spain
13.Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada
14.Univ Basel, Dept Phys, CH-4056 Basel, Switzerland
15.Univ Texas, McDonald Observ, Ft Davis, TX 79734 USA
16.Univ Edinburgh, Inst Astron, Edinburgh EH9 3HJ, Midlothian, Scotland
17.European So Observ, D-85748 Garching, Germany
18.Ctr Hispano Aleman de Calar Alto, Almeria 04004, Spain
19.Chinese Acad Sci, Purple Mt Observ, Natl Astron Observ, Nanjing 210008, Jiangsu, Peoples R China
Recommended Citation
GB/T 7714
Boehm, A.,Wisotzki, L.,Bell, E. F.,et al. AGN host galaxies at redshift z approximate to 0.7: peculiar or not?[J]. ASTRONOMY & ASTROPHYSICS,2013,549:A46-A46.
APA Boehm, A..,Wisotzki, L..,Bell, E. F..,Jahnke, K..,Wolf, C..,...&Zheng, X..(2013).AGN host galaxies at redshift z approximate to 0.7: peculiar or not?.ASTRONOMY & ASTROPHYSICS,549,A46-A46.
MLA Boehm, A.,et al."AGN host galaxies at redshift z approximate to 0.7: peculiar or not?".ASTRONOMY & ASTROPHYSICS 549(2013):A46-A46.
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