activity
20182021
most citedThe SAMI Galaxy Survey: Data Release Two with absorption-line physics value-added products

95 citations · 488 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2021★ 34 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.GA2021★ 48 cited

The SAMI Galaxy Survey: stellar population and structural trends across the Fundamental Plane

Francesco D'Eugenio, Matthew Colless, Nicholas Scott +16

We study the Fundamental Plane (FP) for a volume- and luminosity-limited sample of 560 early-type galaxies from the SAMI survey. Using r-band sizes and luminosities from new Multi-…

astro-ph.GA2021★ 32 cited

A SAMI and MaNGA view on the stellar kinematics of galaxies on the star-forming main sequence

A. Fraser-McKelvie, L. Cortese, J. van de Sande +14

Galaxy internal structure growth has long been accused of inhibiting star formation in disc galaxies. We investigate the potential physical connection between the growth of dispers…

astro-ph.GA2020★ 45 cited

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…

astro-ph.GA2020★ 42 cited

The SAMI Galaxy Survey: A Range in S0 Properties Indicating Multiple Formation Pathways

Simon Deeley, Michael J. Drinkwater, Sarah M. Sweet +14

It has been proposed that S0 galaxies are either fading spirals or the result of galaxy mergers. The relative contribution of each pathway, and the environments in which they occur…

astro-ph.GA2019★ 6 cited

The SAMI Galaxy Survey: rules of behaviour for spin-ellipticity radial tracks in galaxies

Alexander Rawlings, Caroline Foster, Jesse van de Sande +18

We study the behaviour of the spin-ellipticity radial tracks for 507 galaxies from the Sydney AAO Multi-object Integral Field (SAMI) Galaxy Survey with stellar kinematics out to $\…

astro-ph.GA2019★ 30 cited

The SAMI Galaxy Survey: mass-kinematics scaling relations

Dilyar Barat, Francesco D'Eugenio, Matthew Colless +17

We use data from the Sydney-AAO Multi-object Integral-field spectroscopy (SAMI) Galaxy Survey to study the dynamical scaling relation between galaxy stellar mass and the gene…

astro-ph.GA2019★ 45 cited

The SAMI Galaxy Survey: Stellar population radial gradients in early-type galaxies

I. Ferreras, N. Scott, F. La Barbera +16

We study the internal radial gradients of the stellar populations in a sample comprising 522 early-type galaxies (ETGs) from the SAMI (Sydney- AAO Multi-object Integral field spect…

astro-ph.GA2019★ 18 cited

The SAMI Galaxy Survey: Bayesian Inference for Gas Disk Kinematics using a Hierarchical Gaussian Mixture Model

Mathew R. Varidel, Scott M. Croom, Geraint F. Lewis +20

We present a novel Bayesian method, referred to as Blobby3D, to infer gas kinematics that mitigates the effects of beam smearing for observations using Integral Field Spectroscopy…

astro-ph.GA2018★ 93 cited

The SAMI Galaxy Survey: comparing 3D spectroscopic observations with galaxies from cosmological hydrodynamical simulations

Jesse van de Sande, Claudia D. P. Lagos, Charlotte Welker +19

Cosmological hydrodynamical simulations are rich tools to understand the build-up of stellar mass and angular momentum in galaxies, but require some level of calibration to observa…

astro-ph.GA2018★ 95 cited

The SAMI Galaxy Survey: Data Release Two with absorption-line physics value-added products

Nicholas Scott, Jesse van de Sande, Scott M. Croom +34

We present the second major release of data from the SAMI Galaxy Survey. Data Release Two includes data for 1559 galaxies, about 50% of the full survey. Galaxies included have a re…