Statistical analysis of the radio properties of a large sample of 374 optically selected quasars

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/5564

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DC Field	Value	Language
dc.contributor.author	Gopal-Krishna	-
dc.contributor.author	Steppe, H.	-
dc.contributor.author	Ghosh, T.	-
dc.contributor.author	Saripalli, Lakshmi	-
dc.date.accessioned	2013-04-25T06:21:17Z	-
dc.date.available	2013-04-25T06:21:17Z	-
dc.date.issued	1986	-
dc.identifier.citation	IAU Symposium, 1986, Vol.119, p111	en
dc.identifier.uri	http://hdl.handle.net/2289/5564	-
dc.description	Open Access	en
dc.description.abstract	Using a large, unbiased sample of 374 optically selected QSOs, of which 54 are radio detected, the authors have computed for different redshift ranges the probability distribution function ψ(R) of R defined as the ratio of monochromatic luminosities at 15 GHz and 2500 Å in the QSO's rest frame. A significant variation of ψ(R) with redshift is noticed.	en
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1986IAUS..119..111G	en
dc.rights	1986 International Astronomical Union	en
dc.title	Statistical analysis of the radio properties of a large sample of 374 optically selected quasars	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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