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http://hdl.handle.net/2289/5564
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DC Field | Value | Language |
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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) |
Files in This Item:
File | Description | Size | Format | |
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1986_IAUS_V119_p111.pdf Restricted Access | Open Access | 212.84 kB | Adobe PDF | View/Open Request a copy |
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