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

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Sept 2006 An Alternative: Tracing the <strong>Stellar</strong> <strong>Mass</strong> Build-up Directly •Need observations in rest-frame optical/NIR •Measures “older” light •More sensitive to lower mass stars •less IMF dependence •Less affected by extinction •Must observe in near-IR/MIR Berkeley – Gregory Rudnick
Sept 2006 What have deep NIR surveys told us about the galaxy population at high redshift? Berkeley – Gregory Rudnick
Page 1 and 2: Massive Galaxies, the Mean SED, and
Page 3 and 4: Sept 2006 How do Galaxies Grow? Ber
Page 5 and 6: Sept 2006 How do Galaxies Grow? Ber
Page 7: Observing the buildup of stellar ma
Page 11 and 12: The most common massive galaxy at 2
Page 13 and 14: Queiscent Massive Galaxies Sept 200
Page 15 and 16: Sept 2006 Field-to-field Variance H
Page 17 and 18: How to address Science Questions
Page 19 and 20: Sept 2006 Volume Averaged rest-fram
Page 21: Sept 2006 The benefits of averaging
Page 24 and 25: Sept 2006 Observed ρ * Evolution B
Page 26: Sept 2006 Conclusions • Volume av

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