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

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Sept 2006

Detailed Characteristics

Labbé et al. (2005)

Berkeley – Gregory Rudnick

• More massive and older

than UV-selected galaxies

• Some are consistent

with being quiescent

•confirmed by NIR

spectroscopy

(Kriek et al. 2006)

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Sept 2006 Detailed Characteristics Labbé et al. (2005) Berkeley – Gregory Rudnick • More massive and older than UV-selected galaxies • Some are consistent with being quiescent •confirmed by NIR spectroscopy (Kriek et al. 2006)

Queiscent Massive Galaxies Sept 2006 Berkeley – Gregory Rudnick 9 out of 20 K

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 and 8: Observing the buildup of stellar ma
Page 9 and 10: Sept 2006 What have deep NIR survey
Page 11: The most common massive galaxy at 2
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

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

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