506 citations · 3.7k across the 109 of their papers we have counts for
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The SAMI Galaxy Survey: bulge and disk stellar population properties in cluster galaxies
S. Barsanti, M. S. Owers, R. M. McDermid +14
We explore stellar population properties separately in the bulge and the disk of double-component cluster galaxies to shed light on the formation of lenticular galaxies in dense en…
Environmental processing of galaxies in HI-rich groups
Robert Džudžar, Virginia Kilborn, Sarah M. Sweet +3
We present and explore the resolved atomic hydrogen (HI) content of 13 HI-rich and late-type dominated groups denoted `Choirs'. We quantify the HI content of the Choir galaxies wit…
The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework
C. Foster, J. T. Mendel, C. D. P. Lagos +40
We present an overview of the Middle Ages Galaxy Properties with Integral Field Spectroscopy (MAGPI) survey, a Large Program on ESO/VLT. MAGPI is designed to study the physical dri…
The SAMI Galaxy Survey: a statistical approach to an optimal classification of stellar kinematics in galaxy surveys
Jesse van de Sande, Sam P. Vaughan, Luca Cortese +22
Large galaxy samples from multi-object IFS surveys now allow for a statistical analysis of the z~0 galaxy population using resolved kinematics. However, the improvement in number s…
Phase A Science Case for MAVIS -- The Multi-conjugate Adaptive-optics Visible Imager-Spectrograph for the VLT Adaptive Optics Facility
Richard M. McDermid, Giovanni Cresci, Francois Rigaut +18
We present the Phase A Science Case for the Multi-conjugate Adaptive-optics Visible Imager-Spectrograph (MAVIS), planned for the Adaptive Optics Facility (AOF) of the Very Large Te…
SHDE: Survey description and mass-kinematics scaling relations for dwarf galaxies
Dilyar Barat, Francesco D'Eugenio, Matthew Colless +3
The Study of H from Dwarf Emissions (SHDE) is a high spectral resolution (R=13500) H integral field survey of 69 dwarf galaxies with stellar masses $10^6<M_\star<10^9 \,\r…