activity
20162022
most citedThe SAMI Galaxy Survey: the third and final data release

119 citations · 250 across the 8 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2022

The SAMI Galaxy Survey: The Link Between [/Fe] and Kinematic Morphology

Peter J. Watson, Roger L. Davies, Jesse van de Sande +16

We explore a sample of 1492 galaxies with measurements of the mean stellar population properties and the spin parameter proxy, , drawn from the SAMI Galaxy Survey.…

astro-ph.GA202134 cited

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…

astro-ph.GA202117 cited

The SAMI Galaxy Survey: The role of disc fading and progenitor bias in kinematic transitions

S. M. Croom, D. S. Taranu, J. van de Sande +16

We use comparisons between the SAMI Galaxy Survey and equilibrium galaxy models to infer the importance of disc fading in the transition of spirals into lenticular (S0) galaxies. T…

astro-ph.GA2021119 cited

The SAMI Galaxy Survey: the third and final data release

Scott M. Croom, Matt S. Owers, Nicholas Scott +38

We have entered a new era where integral-field spectroscopic surveys of galaxies are sufficiently large to adequately sample large-scale structure over a cosmologically significant…

astro-ph.GA2020

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…

astro-ph.GA2020

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…