activity
20042018
most citedThe SAMI Galaxy Survey: instrument specification and target selection

506 citations · 4.1k across the 42 of their papers we have counts for

collaborators

42 papers

astro-ph.GA2018★ 55 cited

The SAMI Galaxy Survey: Observing the environmental quenching of star formation in GAMA groups

A. L. Schaefer, S. M. Croom, N. Scott +25

We explore the radial distribution of star formation in galaxies in the SAMI Galaxy Survey as a function of their local group environment. Using a sample of galaxies in groups (wit…

astro-ph.GA2018★ 42 cited

KROSS-SAMI: A Direct IFS Comparison of the Tully-Fisher Relation Across 8 Gyr Since

A. L. Tiley, M. Bureau, L. Cortese +27

We construct Tully-Fisher relations (TFRs), from large samples of galaxies with spatially-resolved H emission maps from the K-band Multi-Object Spectrograph (KMOS) Redshift One…

astro-ph.GA2018★ 27 cited

The SAMI Galaxy Survey: gas content and interaction as the drivers of kinematic asymmetry

J. V. Bloom, S. M. Croom, J. J. Bryant +21

In order to determine the causes of kinematic asymmetry in the H gas in the SAMI Galaxy Survey sample, we investigate the comparative influences of environment and intrinsic pro…

astro-ph.GA2018★ 117 cited

The SAMI Galaxy Survey: Spatially Resolving the Main Sequence of Star Formation

Anne M. Medling, Luca Cortese, Scott M. Croom +42

We present the ~800 star formation rate maps for the SAMI Galaxy Survey based on Hα emission maps, corrected for dust attenuation via the Balmer decrement, that are included in the…

astro-ph.GA2017★ 25 cited

The SAMI Galaxy Survey: The Low-Redshift Stellar Mass Tully-Fisher Relation

J. V. Bloom, S. M. Croom, J. J. Bryant +22

We investigate the Tully-Fisher Relation (TFR) for a morphologically and kine- matically diverse sample of galaxies from the SAMI Galaxy Survey using 2 dimensional spatially resolv…

astro-ph.GA2017★ 17 cited

Self-consistent bulge/disk/halo galaxy dynamical modeling using integral field kinematics

D. S. Taranu, D. Obreschkow, J. J. Dubinski +26

We introduce a method for modeling disk galaxies designed to take full advantage of data from integral field spectroscopy (IFS). The method fits equilibrium models to simultaneousl…