The evolution of optically selected quasars with Z less than 2.2 and B less than 20

Astronomy and Astrophysics – Astronomy

Scientific paper

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Luminosity, Quasars, Red Shift, Cosmology, Evolution (Development), Ultraviolet Astronomy

Scientific paper

Several complete samples of optically selected quasars are combined to give details of the quasar luminosity function and its evolution for redshifts less than 2.2. Sufficient coverage of the Hubble diagram is obtained that luminosity-dependent evolution models can be tested and compared against pure luminosity evolution models. Although luminosity-dependent evolution is indicated if the evolution function has an exponential form, the data are consistent with a power-law evolution model that is independent of luminosity. When the sample is split into halves by redshift, a better fit is obtained with a power-law evolution model than with an exponential model. Furthermore, the luminosity function is consistent with a power-law shape whose slope is independent of redshift. The results suggest that the same mass supply and energy generation mechanisms apply over several decades of optical luminosity and for z less than 2.2.

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