Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, Stellar, planetary, and galactic studies, and Gamma-ray bursts and supernovae.
The WiggleZ Dark Energy Survey: The growth rate of cosmic structure since redshift z=0.9
The WiggleZ Dark Energy Survey: Testing the cosmological model with baryon acoustic oscillations at z= 0.6
Measures of galaxy environment - I. What is ‘environment’?
The WiggleZ Dark Energy Survey: high-resolution kinematics of luminous star-forming galaxies
Characterizing tidal features around galaxies in cosmological simulations
The SAMI Galaxy Survey: galaxy spin is more strongly correlated with stellar population age than mass or environment
Preparing for low surface brightness science with the Vera C. Rubin Observatory: a comparison of observable and simulated intracluster light fractions
Galaxy And Mass Assembly (GAMA): Data Release 4 and the <i>z</i> &lt; 0.1 total and <i>z</i> &lt; 0.08 morphological galaxy stellar mass functions
Preparing for low surface brightness science with the Vera C. Rubin Observatory: Characterization of tidal features from mock images
The SAMI Galaxy Survey: The Internal Orbital Structure and Mass Distribution of Passive Galaxies from Triaxial Orbit-superposition Schwarzschild Models
The LEGA-C and SAMI galaxy surveys: quiescent stellar populations and the mass–size plane across 6 Gyr
The SAMI Galaxy Survey: the third and final data release
The SAMI Galaxy Survey: a statistical approach to an optimal classification of stellar kinematics in galaxy surveys
The SAMI galaxy survey: Mass and environment as independent drivers of galaxy dynamics
The LEGA-C and SAMI Galaxy Surveys: Quiescent Stellar Populations and the Mass-Size Plane across 6 Gyr
The SAMI Galaxy Survey: the drivers of gas and stellar metallicity differences in galaxies
The SAMI galaxy survey: exploring the gas-phase mass–metallicity relation
The SAMI Galaxy Survey: Quenching of Star Formation in Clusters I. Transition Galaxies
Galaxy And Mass Assembly (GAMA): Environmental Quenching of Centrals and Satellites in Groups
The SAMI Galaxy Survey: spatially resolving the main sequence of star formation
The SAMI Galaxy Survey: Data Release Two with absorption-line physics value-added products
The SAMI Galaxy Survey: Spatially resolved metallicity and ionization mapping
The SAMI Galaxy Survey: comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations
The SAMI Galaxy Survey: stellar and gas misalignments and the origin of gas in nearby galaxies
A relation between the characteristic stellar ages of galaxies and their intrinsic shapes
Studying galaxy troughs and ridges using weak gravitational lensing with the Kilo-Degree Survey
The SAMI Galaxy Survey: Gravitational Potential and Surface Density Drive Stellar Populations. I. Early-type Galaxies
The SAMI Galaxy Survey: observing the environmental quenching of star formation in GAMA groups
Galaxy and Mass Assembly (GAMA): variation in galaxy structure across the green valley
Galaxy And Mass Assembly: the G02 field, Herschel–ATLAS target selection and data release 3