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The BLR structure and dust torus size of AGN - Implications from photometric and dust reverberation mapping campaigns.
Nunez, F. Pozo1; Ramolla, M.1; Westhues, C.1; Haas, M.1; Chini, R.1,2; Steenbrugge, K.2,3; Lemke, R.1; Murphy, M.2
通讯作者Nunez, F. Pozo
会议名称Workshop on Observing Techniques, Instrumentation and Science for Metre-Class Telescopes
会议日期SEP 23-26, 2013
会议地点Stara Lesna, SLOVAKIA
英文摘要

Photometric reverberation mapping (PRM) is a novel method used to study the geometry of the broad emission-line region (BLR), black hole masses and host-subtracted luminosities of active galactic nuclei (AGN). We obtained high-quality sampling data with small (15 to 80 cm) robotic telescopes at the observatory of the Ruhr-University Bochum, located in the Atacama desert in Chile.


英文关键词galaxies: active galaxies: Seyfert quasars: emission lines galaxies: distances and redshifts galaxies: individual: ESO399-IG20 galaxies: individual: 3C120 galaxies: individual: WPVS48
来源出版物CONTRIBUTIONS OF THE ASTRONOMICAL OBSERVATORY SKALNATE PLESO
ISSN1335-1842
EISSN1336-0337
出版年2014
卷号43
期号3
页码357-361
出版者SLOVAK ACADEMY SCIENCES ASTRONOMICAL INST
类型Article;Proceedings Paper
语种英语
国家Germany;Chile;England
收录类别SCI-E ; CPCI-S
WOS记录号WOS:000338483100032
WOS关键词ACTIVE GALACTIC NUCLEI ; BROAD-LINE REGION
WOS类目Astronomy & Astrophysics
WOS研究方向Astronomy & Astrophysics
资源类型会议论文
条目标识符http://119.78.100.177/qdio/handle/2XILL650/303371
作者单位1.Ruhr Univ Bochum, Astronom Inst, D-44801 Bochum, Germany;
2.Univ Catolica Norte, Inst Astron, Antofagasta 1280, Chile;
3.Univ Oxford, Dept Phys, Oxford OX1 3RH, England
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Nunez, F. Pozo,Ramolla, M.,Westhues, C.,et al. The BLR structure and dust torus size of AGN - Implications from photometric and dust reverberation mapping campaigns.[C]:SLOVAK ACADEMY SCIENCES ASTRONOMICAL INST,2014:357-361.
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