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Frank van den Bosch

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Halo Mass Depen<strong>den</strong>ce<br />

The fractions of early and late type galaxies depend strongly on halo mass.<br />

At fixed halo mass, there is virtually no luminosity depen<strong>den</strong>ce.<br />

The mass depen<strong>den</strong>ce is smooth: there is no characteristic mass scale; i.e.,<br />

no indication that something special happens at the group or cluster scales.<br />

The intermediate type fraction is indepen<strong>den</strong>t of luminosity and mass.<br />

(Weinmann, vdB, Yang & Mo, 2005)

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