K-CLASH: spatially resolving star-forming galaxies in field and cluster environments at z ≈ 0.2–0.6
| dc.contributor.author | Jarvis, Matt | |
| dc.contributor.author | Tiley, Alfred L. | |
| dc.contributor.author | Vaughan, Sam P. | |
| dc.date.accessioned | 2021-02-15T08:46:33Z | |
| dc.date.available | 2021-02-15T08:46:33Z | |
| dc.date.issued | 2020 | |
| dc.description.abstract | We present the KMOS-CLASH (K-CLASH) survey, a K-band Multi-Object Spectrograph (KMOS) survey, of the spatially resolved gas properties and kinematics of 191 (pre-dominantly blue) H α-detected galaxies at 0.2 ≲ z ≲ 0.6 in field and cluster environments. K-CLASH targets galaxies in four Cluster Lensing And Supernova survey with Hubble (CLASH) fields in the KMOS IZ-band, over 7 arcmin radius (≈2–3 Mpc) fields of view. K-CLASH aims to study the transition of star-forming galaxies from turbulent, highly star-forming disc-like and peculiar systems at z ≈ 1–3, to the comparatively quiescent, ordered late-type galaxies at z ≈ 0, and to examine the role of clusters in the build-up of the red sequence since z ≈ 1. | en_US |
| dc.identifier.citation | Jarvis, M. et al. (2020). K-CLASH: spatially resolving star-forming galaxies in field and cluster environments at z ≈ 0.2–0.6. Monthly Notices of the Royal Astronomical Society, 496(1), 649–675 | en_US |
| dc.identifier.issn | 1365-2966 | |
| dc.identifier.uri | https://doi.org/10.1093/mnras/staa1418 | |
| dc.identifier.uri | http://hdl.handle.net/10566/5920 | |
| dc.language.iso | en | en_US |
| dc.publisher | Oxford University Press | en_US |
| dc.subject | Galaxies: evolution | en_US |
| dc.subject | Galaxies: general | en_US |
| dc.subject | Galaxies: kinematics and dynamics | en_US |
| dc.subject | Galaxies: star formation | en_US |
| dc.subject | KMOS-CLASH (K-CLASH) survey | en_US |
| dc.title | K-CLASH: spatially resolving star-forming galaxies in field and cluster environments at z ≈ 0.2–0.6 | en_US |
| dc.type | Article | en_US |