78 citations · 288 across the 7 of their papers we have counts for
7 papers
The WEAVE-LOFAR Survey
D. J. B. Smith, P. N. Best, K. J. Duncan +27
In these proceedings we highlight the primary scientific goals and design of the WEAVE-LOFAR survey, which will use the new WEAVE spectrograph on the 4.2m William Herschel Telescop…
Radial gradients in initial mass function sensitive absorption features in the Coma brightest cluster galaxies
Simon Zieleniewski, Ryan C. W. Houghton, Niranjan Thatte +2
Using the Oxford Short Wavelength Integral Field specTrograph (SWIFT), we trace radial variations of initial mass function (IMF) sensitive absorption features of three galaxies in…
The most massive galaxies in clusters are already fully grown at
L. J. Oldham, R. C. W. Houghton, Roger L. Davies
By constructing scaling relations for galaxies in the massive cluster MACSJ0717.5 at and comparing with those of Coma, we model the luminosity evolution of the stellar po…
The SAMI Pilot Survey: The Kinematic Morphology-Density Relation in Abell 85, Abell 168 and Abell 2399
L. M. R. Fogarty, Nicholas Scott, Matt S. Owers +17
We examine the kinematic morphology of early-type galaxies (ETGs) in three galaxy clusters Abell 85, 168 and 2399. Using data from the Sydney-AAO Multi-object Integral field spectr…
Distribution of Slow and Fast Rotators in the Fornax Cluster
Nicholas Scott, Roger L Davies, Ryan C W Houghton +3
We present integral field spectroscopy of 10 early-type galaxies in the nearby, low-mass, Fornax cluster, from which we derive spatially resolved stellar kinematics. Based on the m…
Fast and slow rotators in the densest environments: a FLAMES/GIRAFFE IFS study of galaxies in Abell 1689 at z=0.183
F. D'Eugenio, R. C. W. Houghton, R. L. Davies +1
We present FLAMES/GIRAFFE integral field spectroscopy of 30 galaxies in the massive cluster Abell 1689 at z = 0.183. Conducting an analysis similar to that of ATLAS3D, we extend th…