{ "id": "1606.00528", "version": "v1", "published": "2016-06-02T03:21:35.000Z", "updated": "2016-06-02T03:21:35.000Z", "title": "ZFIRE: The Kinematics of Star-Forming Galaxies as a Function of Environment at z~2", "authors": [ "Leo Y. Alcorn", "Kim-Vy H. Tran", "Glenn G. Kacprzak", "Themiya Nanayakkara", "Caroline Straatman", "Tiantian Yuan", "Rebecca J. Allen", "Michael Cowley", "Romeel Davé", "Karl Glazebrook", "Lisa J. Kewley", "Ivo Labbé", "Ryan Quadri", "Lee R. Spitler", "Adam Tomczak" ], "comment": "6 pages, 4 figures, accepted for publication in ApJL", "categories": [ "astro-ph.GA" ], "abstract": "We perform a kinematic analysis of galaxies at $z\\sim2$ in the COSMOS legacy field using near-infrared (NIR) spectroscopy from Keck/MOSFIRE as part of the ZFIRE survey. Our sample consists of 75 Ks-band selected star-forming galaxies from the ZFOURGE survey with stellar masses ranging from log(M$_{\\star}$/M$_{\\odot}$)$=9.0-11.0$, 28 of which are members of a known overdensity at $z=2.095$. We measure H$\\alpha$ emission-line integrated velocity dispersions ($\\sigma_{\\rm int}$) from 50$-$230 km s$^{-1}$, consistent with other emission-line studies of $z\\sim2$ field galaxies. From these data we estimate virial, stellar, and gas masses and derive correlations between these properties for cluster and field galaxies at $z\\sim2$. We find evidence that baryons dominate within the central effective radius. However, we find no statistically significant differences between the cluster and the field, and conclude that the kinematics of star-forming galaxies at $z\\sim2$ are not significantly different between the cluster and field environments.", "revisions": [ { "version": "v1", "updated": "2016-06-02T03:21:35.000Z" } ], "analyses": { "keywords": [ "star-forming galaxies", "field galaxies", "emission-line integrated velocity dispersions", "cosmos legacy field", "baryons dominate" ], "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable" } } }