Frank van den Bosch
Frank van den Bosch
Frank van den Bosch
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Luminosity & Correlation Functions<br />
ccccc • 2dFGRS: More luminous galaxies are more strongly clustered.<br />
ccccc • c ΛCDM: More massive haloes are more strongly clustered.<br />
More luminous galaxies reside in more massive haloes<br />
We assume that the CLF has a Schechter-form, and constrain Φ(L|M)<br />
using the Φ(L) and r0(L) shown above.
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