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

dc.contributor.authorJarvis, Matt
dc.contributor.authorTiley, Alfred L.
dc.contributor.authorVaughan, Sam P.
dc.date.accessioned2021-02-15T08:46:33Z
dc.date.available2021-02-15T08:46:33Z
dc.date.issued2020
dc.identifier.citationJarvis, 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), 649–675en_US
dc.identifier.issn1365-2966
dc.identifier.urihttps://doi.org/10.1093/mnras/staa1418
dc.identifier.urihttp://hdl.handle.net/10566/5920
dc.description.abstractWe 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.language.isoenen_US
dc.publisherOxford University Pressen_US
dc.subjectGalaxies: evolutionen_US
dc.subjectGalaxies: generalen_US
dc.subjectGalaxies: kinematics and dynamicsen_US
dc.subjectGalaxies: star formationen_US
dc.subjectKMOS-CLASH (K-CLASH) surveyen_US
dc.titleK-CLASH: spatially resolving star-forming galaxies in field and cluster environments at z ≈ 0.2–0.6en_US
dc.typeArticleen_US


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