L. Wang, D. Farrah, S. J. Oliver, A. Amblard, J. Bock, A. Conley, A. Cooray, M. Halpern, S. Heinis, E. Ibar, O. Ilbert, R. J. Ivison, G. Marsden, I. G. Roseboom, M. Rowan-Robinson, B. Schulz, A. J. Smith, M. Viero, M. Zemcov
We have constructed an extended halo model (EHM) which relates total stellar mass and star formation rate (SFR) to halo mass (M_h). An empirical relation between the distribution functions of total stellar mass of galaxies and host halo mass, tuned to match data over the range 0.1View original: http://arxiv.org/abs/1203.5828
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