Clustering of EROs from UKIDSS DXS and Pan-STARRS PS1

Kim, J.-W.; Edge, A. C.; Wake, D.A.; Gonzalez-Perez, V.; Baugh, C. M.; Lacey, C. G.

Abstract

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.

Citation

Kim, J., Edge, A. C., Wake, D., Gonzalez-Perez, V., Baugh, C. M., & Lacey, C. G. (2013). Clustering of EROs from UKIDSS DXS and Pan-STARRS PS1. In D. Thomas, A. Pasquali, & I. Ferreras (Eds.), Proceedings IAU Symposium (59-59). https://doi.org/10.1017/s1743921313004298

• Conference Name: IAU Symposium
• Online Publication Date: Jul 17, 2013
• Publication Date: 2013-07
• Deposit Date: May 16, 2014
• Volume: 295
• Pages: 59-59
• Series Title: IAU Symposium
• Series Number: S295
• Series ISSN: 1743-9213
• Book Title: Proceedings IAU Symposium
• DOI: https://doi.org/10.1017/s1743921313004298
• Public URL: https://durham-repository.worktribe.com/output/1155013
• Related Public URLs: http://adsabs.harvard.edu/abs/2013IAUS..295...59K