Jarvis, MattTiley, Alfred L.Vaughan, Sam P.2021-02-152021-02-152020Jarvis, 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), 649–6751365-2966https://doi.org/10.1093/mnras/staa1418http://hdl.handle.net/10566/5920We 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.enGalaxies: evolutionGalaxies: generalGalaxies: kinematics and dynamicsGalaxies: star formationKMOS-CLASH (K-CLASH) surveyArticle