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Efficient satellite quenching at z∼1 from the...
Journal article

Efficient satellite quenching at z∼1 from the GEEC2 spectroscopic survey of galaxy groups

Abstract

We present deep Gemini Multi-Object Spectrograph-South spectroscopy for 11 galaxy groups at 0.8 < z < 1.0, for galaxies with rAB < 24.75. Our sample is highly complete (>66 per cent) for eight of the 11 groups. Using an optical–near-infrared colour–colour diagram, the galaxies in the sample were separated with a dust insensitive method into three categories: passive (red), star-forming (blue) and intermediate (green). The strongest environmental dependence is observed in the fraction of passive galaxies, which make …

Authors

Mok A; Balogh ML; McGee SL; Wilman DJ; Finoguenov A; Tanaka M; Giodini S; Bower RG; Connelly JL; Hou A

Journal

Monthly Notices of the Royal Astronomical Society, Vol. 431, No. 2, pp. 1090–1106

Publisher

Oxford University Press (OUP)

Publication Date

May 11, 2013

DOI

10.1093/mnras/stt251

ISSN

0035-8711