Journal article

K-CLASH: spatially resolving star-forming galaxies in field and cluster environments at z approximate to 0.2-0.6

Alfred L Tiley, Sam P Vaughan, John P Stott, Roger L Davies, Laura J Prichard, Andrew Bunker, Martin Bureau, Michele Cappellari, Matt Jarvis, Aaron Robotham, Luca Cortese, Sabine Bellstedt, Behzad Ansarinejad

Monthly Notices of the Royal Astronomical Society | Royal Astronomical Society | Published : 2020


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..

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University of Melbourne Researchers