K-CLASH: spatially resolving star-forming galaxies in field and cluster environments at z ≈ 0.2–0.6. Issue 1 (22nd May 2020)

• Record Type: Journal Article
• Authors: Tiley, Alfred L; Vaughan, Sam P; Stott, John P; Davies, Roger L; Prichard, Laura J; Bunker, Andrew; Bureau, Martin; Cappellari, Michele; Jarvis, Matt; Robotham, Aaron; Cortese, Luca; Bellstedt, Sabine; Ansarinejad, Behzad
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 496:Issue 1(2020)
• Page Start: 649
• Page End: 675
• Publication Date: 2020-05-22
• Subjects: galaxies: evolution -- galaxies: general -- galaxies: kinematics and dynamics -- galaxies: star formation; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/staa1418
• Languages: English
• ISSNs: 0035-8711

Abstract

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. In this paper, we describe the K-CLASH survey, present the sample, and provide an overview of the K-CLASH galaxy properties. We demonstrate that our sample comprises star-forming galaxies typical of their stellar masses and epochs, residing both in field and cluster environments. We conclude K-CLASH provides an ideal sample to bridge the gap between existing large integral-field spectroscopy surveys at higher and lower redshifts. We find that star-forming K-CLASH cluster galaxies at intermediate redshifts have systematically lower stellar masses than their star-forming counterparts in the field, hinting at possible 'downsizing' scenarios of galaxy growth in clusters at these epochs. We measure no difference between the star formation rates of H α-detected, star-forming galaxies in either environment after accounting for stellar mass, suggesting that cluster quenching occurs very rapidly during the epochs probed by K-CLASH, or that star-forming K-CLASH galaxies in clusters have only recently arrived there, with insufficient time elapsed for quenching to have occurred.