activity
20072020
most citedThe SAMI Pilot Survey: The Kinematic Morphology-Density Relation in Abell 85, Abell 168 and Abell 2399

78 citations · 837 across the 28 of their papers we have counts for

collaborators
Showing 2016Show all

6 papers · 1 filter

astro-ph.GA2016★ 31 cited

Radial measurements of IMF-sensitive absorption features in two massive ETGs

Sam P. Vaughan, Roger L. Davies, Simon Zieleniewski +1

We make radial measurements of stellar initial mass function (IMF) sensitive absorption features in the two massive early-type galaxies NGC 1277 and IC 843. Using the Oxford Short…

astro-ph.GA2016★ 16 cited

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…

astro-ph.GA2016★ 36 cited

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…

astro-ph.GA2016★ 9 cited

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…

astro-ph.GA2016★ 56 cited

Sizes, Colour gradients and Resolved Stellar Mass Distributions for the Massive Cluster Galaxies in XMMUJ2235-2557 at z = 1.39

Jeffrey C. C. Chan, Alessandra Beifiori, J. Trevor Mendel +13

We analyse the sizes, colour gradients, and resolved stellar mass distributions for 36 massive and passive galaxies in the cluster XMMUJ2235-2557 at z=1.39 using optical and near-i…

astro-ph.GA2016★ 11 cited

Simulated stellar kinematics studies of high-redshift galaxies with the HARMONI Integral Field Spectrograph

S. Kendrew, S. Zieleniewski, R. C. W. Houghton +6

We present a study into the capabilities of integrated and spatially resolved integral field spectroscopy of galaxies at z=2-4 with the future HARMONI spectrograph for the European…