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	The BLR structure and dust torus size of AGN - Implications from photometric and dust reverberation mapping campaigns.
	Nunez, F. Pozo 1; 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
ISSN	1335-1842
EISSN	1336-0337
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/2XILL650/303581
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
推荐引用方式 GB/T 7714	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.