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  • 2005.12471

    Rights statement: This is a pre-copy-editing, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The definitive publisher-authenticated version 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, 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, Volume 496, Issue 1, July 2020, Pages 649–675, https://doi.org/10.1093/mnras/staa1418 is available online at: https://academic.oup.com/mnras/article/496/1/649/5841949

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

In: Monthly Notices of the Royal Astronomical Society, Vol. 496, No. 1, 01.07.2020, p. 649-675.

Research output: Contribution to journalJournal articlepeer-review

Harvard

Tiley, AL, Vaughan, SP, Stott, JP, Davies, RL, Prichard, LJ, Bunker, A, Bureau, M, Cappellari, M, Jarvis, M, Robotham, A, Cortese, L, Bellstedt, S & Ansarinejad, B 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, vol. 496, no. 1, pp. 649-675. https://doi.org/10.1093/mnras/staa1418

APA

Tiley, A. L., Vaughan, S. P., Stott, J. P., Davies, R. L., Prichard, L. J., Bunker, A., Bureau, M., Cappellari, M., Jarvis, M., Robotham, A., Cortese, L., Bellstedt, S., & Ansarinejad, B. (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), 649-675. https://doi.org/10.1093/mnras/staa1418

Vancouver

Tiley AL, Vaughan SP, Stott JP, Davies RL, Prichard LJ, Bunker A et al. 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. 2020 Jul 1;496(1):649-675. https://doi.org/10.1093/mnras/staa1418

Author

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. / K-CLASH: spatially resolving star-forming galaxies in field and cluster environments at z ≍ 0.2–0.6. In: Monthly Notices of the Royal Astronomical Society. 2020 ; Vol. 496, No. 1. pp. 649-675.

Bibtex

@article{a73d4ed0ac804eaa95e9a789f3d657f4,
title = "K-CLASH: spatially resolving star-forming galaxies in field and cluster environments at z ≍ 0.2–0.6",
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.",
keywords = "galaxies: star formation, galaxies: evolution, galaxies: general, galaxies: kinematics and dynamics",
author = "Tiley, {Alfred L.} and Vaughan, {Sam P.} and Stott, {John P.} and Davies, {Roger L.} and Prichard, {Laura J.} and Andrew Bunker and Martin Bureau and Michele Cappellari and Matt Jarvis and Aaron Robotham and Luca Cortese and Sabine Bellstedt and Behzad Ansarinejad",
note = "This is a pre-copy-editing, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The definitive publisher-authenticated version 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, 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, Volume 496, Issue 1, July 2020, Pages 649–675, https://doi.org/10.1093/mnras/staa1418 is available online at: https://academic.oup.com/mnras/article/496/1/649/5841949",
year = "2020",
month = jul,
day = "1",
doi = "10.1093/mnras/staa1418",
language = "English",
volume = "496",
pages = "649--675",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "OXFORD UNIV PRESS",
number = "1",

}

RIS

TY - JOUR

T1 - K-CLASH: spatially resolving star-forming galaxies in field and cluster environments at z ≍ 0.2–0.6

AU - Tiley, Alfred L.

AU - Vaughan, Sam P.

AU - Stott, John P.

AU - Davies, Roger L.

AU - Prichard, Laura J.

AU - Bunker, Andrew

AU - Bureau, Martin

AU - Cappellari, Michele

AU - Jarvis, Matt

AU - Robotham, Aaron

AU - Cortese, Luca

AU - Bellstedt, Sabine

AU - Ansarinejad, Behzad

N1 - This is a pre-copy-editing, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The definitive publisher-authenticated version 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, 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, Volume 496, Issue 1, July 2020, Pages 649–675, https://doi.org/10.1093/mnras/staa1418 is available online at: https://academic.oup.com/mnras/article/496/1/649/5841949

PY - 2020/7/1

Y1 - 2020/7/1

N2 - 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.

AB - 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.

KW - galaxies: star formation

KW - galaxies: evolution

KW - galaxies: general

KW - galaxies: kinematics and dynamics

U2 - 10.1093/mnras/staa1418

DO - 10.1093/mnras/staa1418

M3 - Journal article

VL - 496

SP - 649

EP - 675

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 1

ER -