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20012017
most citedThe KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z~0.9 galaxies

99 citations · 280 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2017★ 99 cited

The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z~0.9 galaxies

C. M. Harrison, H. L. Johnson, A. M. Swinbank +12

We present dynamical measurements for 586 H-alpha detected star-forming galaxies from the KMOS (K-band Multi-Object Spectrograph) Redshift One Spectroscopic Survey (KROSS). The sam…

astro-ph.GA2016★ 9 cited

The Spatially Resolved Dynamics of Dusty Starburst Galaxies in a z ~ 0.4 Cluster: Beginning the Transition from Spirals to S0s

H. L. Johnson, C. M. Harrison, A. M. Swinbank +4

To investigate what drives the reversal of the morphology-density relation at intermediate/high redshift, we present a multi-wavelength analysis of 27 dusty starburst galaxies in t…

astro-ph.CO2009★ 39 cited

Dissecting the Lyman Alpha Emission Halo of LAB1

A. Weijmans, R. G. Bower, J. E. Geach +4

We report observations of Lyman Alpha Blob 1 (LAB1) in the SSA 22 protocluster region (z=3.09) with the integral-field spectrograph SAURON. We increased the signal-to-noise in the…

astro-ph2004★ 19 cited

GMOS Integral Field Spectroscopy of a Merging System with Enhanced Balmer Absorption

Mark Swinbank, Michael Balogh, Richard Bower +4

In this paper we present the three dimensional dynamics of the galaxy SDSS J101345.39+011613.66, selected for its unusually strong Balmer absorption lines (Wo(H-delta)=7.5A). Using…

astro-ph2002★ 62 cited

Galaxy Properties in Low X-Ray Luminosity Clusters at z=0.25

Michael L. Balogh, R. G. Bower, Ian Smail +4

We present the first spectroscopic survey of intrinsically low Lx clusters at z>>0, with HST WFPC2 imaging and ground-based spectroscopy. We study 172 confirmed cluster members in…

astro-ph2002

Galaxy Evolution: Internally or Externally Driven?

M. L. Balogh, R. G. Bower

The globally-averaged star formation rate in the Universe has been steadily declining since at least z~1. This may be due either to very local processes operating within the averag…