Galaxy formation in the Planck cosmology – I. Matching the observed evolution of star formation rates, colours and stellar masses

We have updated the Munich galaxy formation model to the Planck first-year cosmology, while modifying the treatment of baryonic processes to reproduce recent data on the abundance and passive fractions of galaxies from z = 3 down to z = 0. Matching these more extensive and more precise observational...

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Bibliographic Details
Published in:	Monthly notices of the Royal Astronomical Society 2015-08, Vol.451 (3), p.2663-2680
Main Authors:	Henriques, Bruno M. B., White, Simon D. M., Thomas, Peter A., Angulo, Raul, Guo, Qi, Lemson, Gerard, Springel, Volker, Overzier, Roderik
Format:	Article
Language:	English
Subjects:	Astronomy Cosmology Formations Galaxy formation Matching Mathematical models Star & galaxy formation Star formation rate Stars Stellar mass
Citations:	Items that this one cites Items that cite this one
Online Access:	Request full text
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