Clustering of EROs from UKIDSS DXS and Pan-STARRS PS1
The Intriguing Life of Massive Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 295, pp. 59-59
Published in Jul 2013
We have measured the angular two-point correlation function of EROs. The halo model is fitted to the observed clustering, and dark matter halo mass, bias and satellite fraction are estimated in three redshift bins. We also compare our results with the semi-analytical galaxy formation model. This work illustrates the power of clustering analysis in providing observational constraints on simulations.
galaxies: halos; infrared: galaxies; large-scale structure
(c) 2013: Copyright © International Astronomical Union 2013