ZFIRE: The kinematics of star-forming galaxies as a function of environment at z ∼ 2
Article
Alcorn, Leo Y., Tran, Kim-Vy H., Kacprzak, Glenn G., Nanayakkara, Themiya, Straatman, Caroline, Yuan, Tiantian, Allen, Rebecca J., Cowley, Michael, Davé, Romeel, Glazebrook, Karl, Kewley, Lisa J., Labbé, Ivo, Quadri, Ryan, Spitler, Lee R. and Tomczak, Adam. 2016. "ZFIRE: The kinematics of star-forming galaxies as a function of environment at z ∼ 2." The Astrophysical Journal Letters. 825 (1), pp. 1-6. https://doi.org/10.3847/2041-8205/825/1/L2
| Article Title | ZFIRE: The kinematics of star-forming galaxies as a function of environment at z ∼ 2 |
|---|---|
| ERA Journal ID | 45091 |
| Article Category | Article |
| Authors | Alcorn, Leo Y., Tran, Kim-Vy H., Kacprzak, Glenn G., Nanayakkara, Themiya, Straatman, Caroline, Yuan, Tiantian, Allen, Rebecca J., Cowley, Michael, Davé, Romeel, Glazebrook, Karl, Kewley, Lisa J., Labbé, Ivo, Quadri, Ryan, Spitler, Lee R. and Tomczak, Adam |
| Journal Title | The Astrophysical Journal Letters |
| Journal Citation | 825 (1), pp. 1-6 |
| Article Number | L2 |
| Number of Pages | 6 |
| Year | 2016 |
| Publisher | IOP Publishing |
| Place of Publication | United Kingdom |
| ISSN | 2041-8205 |
| 2041-8213 | |
| Digital Object Identifier (DOI) | https://doi.org/10.3847/2041-8205/825/1/L2 |
| Web Address (URL) | https://iopscience.iop.org/article/10.3847/2041-8205/825/1/L2 |
| Abstract | We perform a kinematic analysis of galaxies at z ∼ 2 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 ∗/M o) = 9.0-11.0, 28 of which are members of a known overdensity at z = 2.095. We measure H emission-line integrated velocity dispersions (σ int) from 50 to 230 km s-1, consistent with other emission-line studies of z ∼ 2 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 ∼ 2. 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 ∼ 2 are not significantly different between the cluster and field environments. |
| Keywords | galaxies: evolution |
| Contains Sensitive Content | Does not contain sensitive content |
| Public Notes | For access to this article, please click on the URL link provided. |
| Funder | National Science Foundation |
| Byline Affiliations | Texas A&M University, United States |
| Swinburne University of Technology | |
| Leiden University, Netherlands | |
| Australian National University | |
| Australian Astronomical Observatory, Australia | |
| Macquarie University | |
| University of the Western Cape, South Africa | |
| South African Astronomical Observatory, South Africa | |
| African Institute for Mathematical Sciences, South Africa | |
| University of California, United States |
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