{ "id": "1605.05314", "version": "v1", "published": "2016-05-17T19:59:35.000Z", "updated": "2016-05-17T19:59:35.000Z", "title": "Differences in the structural properties and star-formation rates of field and cluster galaxies at z~1", "authors": [ "Rebecca J. Allen", "Glenn G. Kacprzak", "Karl Glazebrook", "Kim-Vy H. Tran", "Lee R. Spitler", "Caroline M. S. Straatman", "Michael Cowley", "Themiya Nanayakkara" ], "comment": "13 pages, 10 figures, accepted by Apj", "categories": [ "astro-ph.GA" ], "abstract": "We investigate the dependance of galaxy sizes and star-formation rates (SFRs) on environment using a mass-limited sample of quiescent and star-forming galaxies with M>10^9.5 at z=0.92 selected from the NMBS survey. Using the GEEC2 spectroscopic cluster catalog and the accurate photometric redshifts from NMBS, we select quiescent and star-forming cluster (sigma=490 km/s) galaxies within two virial radius, Rvir, intervals of 0.51, than field star-forming galaxies. The average SFRs of star-forming cluster galaxies show a trend of decreasing SFR with clustocentric radius. The mass-normalised average SFR of cluster star-forming galaxies is a factor of 2-2.5 (7-9 sigma) lower than that of star-forming galaxies in the field. While we find no significant dependence on environment for quiescent galaxies, the properties of star-forming galaxies are affected, which could be the result of environment acting on their gas content.", "revisions": [ { "version": "v1", "updated": "2016-05-17T19:59:35.000Z" } ], "analyses": { "keywords": [ "star-formation rates", "cluster galaxies", "star-forming galaxies", "structural properties", "average sfr" ], "note": { "typesetting": "TeX", "pages": 13, "language": "en", "license": "arXiv", "status": "editable" } } }