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the COSMOS Team

Publications and source records attributed to the COSMOS Team.

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The M*-Mhalo relation at 0.08 < z < 1.53 in COSMOS: the role of AGN radio-mode feedback

In the current picture of cosmology and astrophysics, the formation and evolution of galaxies is closely linked to that of their dark matter haloes. The best representation of this galaxy-dark matter halo co-evolution is the M* - Mhalo relation. In this study we investigate how the radio-mode feedback from active galactic nuclei (AGN) affects the M* - Mhalo relation at redshifts 0.08 < z < 1.53. We use a set of 111 radio-selected AGN at 3 GHz VLA-COSMOS within the X-ray galaxy groups in the COSMOS field. We compare these results to the ones of 171 star-forming galaxies (SFGs), using the theoretical relation of Moster et al. (2013). We find that AGN agree within 1% with the Moster et al. (2013) relation, SFGs show an offset of 37%, suggesting that the radio-mode feedback from AGN at a median redshift of ~ 0.5 still plays a significant role in the M* - Mhalo relation.

astro-ph.GA

The HST Cosmos Project: Contribution from the Subaru Telescope

The Cosmic Evolution Survey (COSMOS) is a Hubble Space Telescope (HST) treasury project.The COSMOS aims to perform a 2 square degree imaging survey of an equatorial field in $I$(F814W) band, using the Advanced Camera for Surveys (ACS). Such a wide field survey, combined with ground-based photometric and spectroscopic data, is essential to understand the interplay between large scale structure, evolution and formation of galaxies and dark matter. In 2004, we have obtained high-quality, broad band images of the COSMOS field ($B, V, r^\prime, i^\prime,$ and $ z^\prime$) using Suprime-Cam on the Subaru Telescope, and we have started our new optical multi-band program, COSMOS-21 in 2005. Here, we present a brief summary of the current status of the COSMOS project together with contributions from the Subaru Telescope. Our future Subaru program, COSMOS-21, is also discussed briefly.

astro-ph