Sravani Vaddi 1, Chris O’Dea 1, Stefi Baum 1, Christine Jones 2, Bill Forman2, Samantha Whitmore 3 and Rabeea Ahmed 3 1 Astrophysical Sciences & Technology,
Galaxy Formation in the Early Universe Haojing Yan Center for Cosmology & AstroParticle Physics Ohio State University CCAPP Symposium 2009 October 14,
1510.08845
Cosmic Variance and Luminosity Function Fitting
The sdss galaxies at redshift 0.1
Galaxy Luminosity Function (LF) – Φ (yes, another use of “ phee ”!)
Galaxy Luminosity Function (LF) – Φ (yes, another use of “phee”!) - What are the relative numbers of galaxies of different luminosities? δN = Φ(L) δL δV.
What can we learn from the luminosity function and color studies? THE SDSS GALAXIES AT REDSHIFT 0.1.
Feedback, Models and the effect of Environment
GRBs as cosmological probes
