Michael Strauss
Michael Strauss
Michael Strauss
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Conclusions<br />
ß SDSS is a tremendously powerful tool for studying the optical<br />
properties of AGN at z=0 to z=6.5.<br />
ß Luminous quasars peaked in comoving space density at z~2.5.<br />
Luminosity function slope change is qualitatively consistent<br />
with ‘cosmic downsizing’ picture.<br />
ß At low redshifts, AGN luminosity function can be pushed<br />
down to very low luminosities. Continuity with classical<br />
quasars is work in progress.<br />
ß Very luminous Type II quasars can be selected from the<br />
SDSS spectroscopic sample, and studied in detail.<br />
ß Ask me about the latest results on quasars at high (z~6)<br />
quasars…
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