594 citations · 10.5k across the 171 of their papers we have counts for
11 papers · 1 filter
The SAMI Galaxy Survey: the drivers of gas and stellar metallicity differences in galaxies
A. Fraser-McKelvie, L. Cortese, B. Groves +13
The combination of gas-phase oxygen abundances and stellar metallicities can provide us with unique insights into the metal enrichment histories of galaxies. In this work, we compa…
Galaxy And Mass Assembly (GAMA): The environmental impact on SFR and metallicity in galaxy groups
D. Sotillo-Ramos, M. A. Lara-Lopez, A. M. Perez-Garcia +7
We present a study of the relationships and environmental dependencies between stellar mass, star formation rate, and gas metallicity for more than 700 galaxies in groups up to red…
The SAMI Galaxy Survey: Mass and Environment as Independent Drivers of Galaxy Dynamics
Jesse van de Sande, Scott M. Croom, Joss Bland-Hawthorn +16
The kinematic morphology-density relation of galaxies is normally attributed to a changing distribution of galaxy stellar masses with the local environment. However, earlier studie…
The LEGA-C and SAMI Galaxy Surveys: Quiescent Stellar Populations and the Mass-Size Plane across 6 Gyr
Tania M. Barone, Francesco D'Eugenio, Nicholas Scott +22
We investigate the change in mean stellar population age and metallicity ([Z/H]) scaling relations for quiescent galaxies from intermediate redshift () using th…
The SAMI Galaxy Survey: Detection of Environmental Dependence of Galaxy Spin in Observations and Simulations Using Marked Correlation Functions
Tomas H. Rutherford, Scott M. Croom, Jesse van de Sande +6
The existence of a kinematic morphology-density relation remains uncertain, and instead stellar mass appears the more dominant driver of galaxy kinematics. We investigate the depen…
The SAMI Galaxy Survey: Trends in [α/Fe] as a Function of Morphology and Environment
Peter J. Watson, Roger L. Davies, Sarah Brough +16
We present a new set of index-based measurements of [/Fe] for a sample of 2093 galaxies in the SAMI Galaxy Survey. Following earlier work, we fit a global relation between [/…