Hard X-ray flux variations in AGN from NuSTAR

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DC Field	Value	Language
dc.contributor.author	Priyanka Rani	-
dc.contributor.author	Stalin, C. S	-
dc.date.accessioned	2020-11-27T01:24:52Z	-
dc.date.available	2020-11-27T01:24:52Z	-
dc.date.issued	2015-04	-
dc.identifier.citation	ASI Conference Series, Vol. 12, pp. 135-136	en_US
dc.identifier.uri	http://prints.iiap.res.in/handle/2248/7472	-
dc.description	Open Access © Astronomical Society of India http://www.astron-soc.in/bulletin/asics_vol012/pdfs/priyanka.pdf	en_US
dc.description.abstract	We present here our results on the hour like time scale Xray flux variations in a sample of active galactic nuclei using data from the Nuclear Spectroscopic Telescope Array (NuSTAR). We find that in the 3−79 keV band, BL Lacs are more variable than flat spectrum radio quasars and Seyfert galaxies. Among Seyferts, Seyfert 2s are more variable than Seyfert 1s. Also, radio-loud quasars are more variable in the hard (10−79 keV) band than the soft (3−10 keV) band while, Seyfert galaxies tend to show more variations in the soft band relative to the hard band.	en_US
dc.language.iso	en	en_US
dc.publisher	Astronomical Society of India	en_US
dc.subject	Galaxies: active	en_US
dc.subject	galaxies:Seyfert	en_US
dc.subject	- BL Lacertae objects:general	en_US
dc.title	Hard X-ray flux variations in AGN from NuSTAR	en_US
dc.type	Article	en_US
Appears in Collections:	IIAP Publications

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