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Michael Strauss

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n 5645 quasars<br />

with g < 21.85<br />

selected from<br />

SDSS imaging,<br />

observed with<br />

2dF at AAT. UV<br />

excess sources,<br />

almost all with z<br />

< 2.5. Best-fit<br />

slope b is -1.45 at<br />

faint end.<br />

A crucial question: the shape and<br />

slope of the LF at the faint end… end<br />

Richards et al. 2005a<br />

MNRAS

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