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The Mean Spectral Energy Distribution and Stellar Mass Density of ...

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Sept 2006<br />

Field-to-field Variance<br />

HDF-N<br />

HDF-S<br />

Cosmic variance in this population<br />

is large.<br />

Berkeley – Gregory Rudnick<br />

• GOODS-S is underdense bv<br />

~2 in number <strong>of</strong> massive z~2<br />

galaxies<br />

Multiple fields needed to measure<br />

their contribution to the mass<br />

density.<br />

Labbé et al. (2003)

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