From fields to a super-cluster:the role of the environment at z=0:84 with HiZELS

Sobral, D. and Best, P. and Smail, I. J. (2011) From fields to a super-cluster:the role of the environment at z=0:84 with HiZELS. In: Environment and the Formation of Galaxies: 30 years later. Astrophysics and Space Science Proceedings . Springer, PRT, pp. 179-184. ISBN 9783642202841

Full text not available from this repository.


At z=0, clusters are primarily populated by red, elliptical and massive galaxies, while blue, spiral and lower-mass galaxies are common in low-density environments. Understanding how and when these differences were established is of absolute importance for our understanding of galaxy formation and evolution, but results at high-z remain contradictory. By taking advantage of the widest and deepest Hα narrow-band survey at z=0:84 over the COSMOS and UKIDSS UDS fields, probing a wide range of densities (from poor fields to rich groups and clusters, including a confirmed super-cluster with a striking filamentary structure), we show that the fraction of star-forming galaxies falls continuously from ∼40% in fields to approaching 0% in rich groups/clusters. We also find that the median SFR increases with environmental density, at least up to group densities - but only for low and medium mass galaxies, and thus such enhancement is mass-dependent at z ∼ 1. The environment also plays a role in setting the faint-end slope (α) of the Hα luminosity function. Our findings provide a sharper view on galaxy formation and evolution and reconcile previously contradictory results at z∼1: stellar mass is the primary predictor of star formation activity, but the environment also plays a major role.

Item Type:
Contribution in Book/Report/Proceedings
Uncontrolled Keywords:
ID Code:
Deposited By:
Deposited On:
15 Jan 2016 16:04
Last Modified:
19 Sep 2023 03:24