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

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    staa1418.pdf (4.546Mb)
    Date
    2020
    Author
    Jarvis, Matt
    Tiley, Alfred L.
    Vaughan, Sam P.
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    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.
    URI
    https://doi.org/10.1093/mnras/staa1418
    http://hdl.handle.net/10566/5920
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    • Research Articles (Physics)

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