The UVX quasar optical luminosity function and its evolution

The UVX quasar optical luminosity function and its evolution

The recently-finished Edinburgh UVX quasar survey at B < 18 is used together with other complete samples to estimate the shape and evolution of the optical luminosity function in the redshift range 0.3 < z < 2.2. There is a significantly higher space density of quasars at high l...

書誌詳細
主要な著者:	Goldschmidt, P, Miller, L
フォーマット:	Journal article
言語:	English
出版事項:	1997

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