THE AVERAGE STAR FORMATION HISTORIES OF GALAXIES IN DARK MATTER HALOS FROM z = 0-8
Kavli Institute for Particle Astrophysics and Cosmology · Stanford University · +2 more institutions
Abstract
We present a robust method to constrain average galaxy star formation rates, star formation histories, and the intracluster light as a function of halo mass. Our results are consistent with observed galaxy stellar mass functions, specific star formation rates, and cosmic star formation rates from z=0 to z=8. We consider the effects of a wide range of uncertainties on our results, including those affecting stellar masses, star formation rates, and the halo mass function at the heart of our analysis. As they are relevant to our method, we also present new calibrations of the dark matter halo mass function, halo mass accretion histories, and halo-subhalo merger rates out to z=8. We also provide new compilations…
Citation impact
- FWCI
- 116.74
- Percentile
- 100%
- References
- 214
Authors
3- PBPeter BehrooziCorresponding
Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, SLAC National Accelerator Laboratory
- RHRisa H. Wechsler
Kavli Institute for Particle Astrophysics and Cosmology, SLAC National Accelerator Laboratory, Stanford University
- CCCharlie Conroy
University of California, Santa Cruz
Topics & keywords
- Astrophysics
- Physics
- Dark matter
- Galaxy
- Astronomy
- Dark matter halo
- Halo