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Brough Sarah
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http://hub.abes.fr/edp/periodical/aa/2012/volume_547/issue_2012/aa20050-12/authorship/18
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Galaxy And Mass Assembly (GAMA): Improved emission lines measurements in four representative samples at 0.07 <z < 0.3
Galaxy And Mass Assembly (GAMA): Galaxy colour gradients versus colour, structure, and luminosity
The WiggleZ Dark Energy Survey: small-scale clustering of Lyman-break galaxies at z< 1
The anatomy of the NGC 5044 group - II. Stellar populations and star formation histories
Environmental dependence of the structure of brightest cluster galaxies
Southern GEMS groups - II. H i distribution, mass functions and H i deficient galaxies
The early-type galaxies NGC 1407 and NGC 1400 - I. Spatially resolved radial kinematics and surface photometry
The WiggleZ Dark Energy Survey: the selection function and z= 0.6 galaxy power spectrum
The anatomy of the NGC 5044 group - I. Group membership and dynamics
The WiggleZ Dark Energy Survey
Gaseous tidal debris found in the NGC 3783 group
The luminosity-halo mass relation for brightest cluster galaxies
Spatially resolved kinematics and stellar populations of brightest cluster and group galaxies
Eridanus - a supergroup in the local Universe?
The early-type galaxies NGC 1407 and NGC 1400 - II. Star formation and chemical evolutionary history
Evolution of brightest cluster galaxies in X ray clusters
The discovery of new galaxy members in the NGC 5044 and 1052 groups
The WiggleZ Dark Energy Survey: survey design and first data release
Galaxy And Mass Assembly (GAMA): the mass-metallicity relationship
Galaxy and Mass Assembly: Group and field galaxy morphologies in the star-formation rate - stellar mass plane
The XXL Survey
G alapagos-2/G alfitm/G ama - Multi-wavelength measurement of galaxy structure: Separating the properties of spheroid and disk components in modern surveys
Photometric redshifts for the Kilo-Degree Survey
Galaxy and Mass Assembly (GAMA): The environmental dependence of the galaxy main sequence
Galaxy and Mass Assembly (GAMA): Accurate number densities and environments of massive ultra-compact galaxies at 0.02 < z< 0.3
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