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

More documents

Recommendations

Info

Sept 2006 How do Galaxies Grow? simulation by volker springel Berkeley – Gregory Rudnick •The initial conditions are well known. •The dark matter paradigm is well developed. •The growth of DM halos can be traced via simulations.
Sept 2006 How do Galaxies Grow? Berkeley – Gregory Rudnick •The initial conditions are well known. •The dark matter paradigm is well developed. •The growth of DM halos can be traced via simulations. •Add baryonic (gastrophysics) physics to DM simulation, e.g.: •star formation, cooling, feedback from SF, feedback from an AGN •From DM to observables!! •But, physics are very uncertain and observational constraints are crucial
Page 1 and 2: Massive Galaxies, the Mean SED, and
Page 3: 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 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

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

Create successful ePaper yourself

Delete template?

Save as template?