activity
20162026
most citedThe SAMI Galaxy Survey: The internal orbital structure and mass distribution of passive galaxies from triaxial orbit-superposition Schwarzschild models

52 citations · 307 across the 33 of their papers we have counts for

collaborators
Showing 2022Show all

5 papers · 1 filter

astro-ph.GA2022★ 10 cited

The SAMI Galaxy Survey: Using concentrated star-formation and stellar population ages to understand environmental quenching

Di Wang, Scott M. Croom, Julia J. Bryant +16

We study environmental quenching using the spatial distribution of current star-formation and stellar population ages with the full SAMI Galaxy Survey. By using a star-formation co…

astro-ph.GA2022★ 37 cited

The SAMI Galaxy Survey: flipping of the spin-filament alignment correlates most strongly with growth of the bulge

Stefania Barsanti, Matthew Colless, Charlotte Welker +8

We study the alignments of galaxy spin axes with respect to cosmic web filaments as a function of various properties of the galaxies and their constituent bulges and discs. We expl…

astro-ph.GA2022★ 3 cited

The SAMI Galaxy Survey: The relationship between galaxy rotation and the motion of neighbours

Yifan Mai, Sam P. Vaughan, Scott M. Croom +12

Using data from the SAMI Galaxy Survey, we investigate the correlation between the projected stellar kinematic spin vector of 1397 SAMI galaxies and the line-of-sight motion of the…

astro-ph.GA2022★ 52 cited

The SAMI Galaxy Survey: The internal orbital structure and mass distribution of passive galaxies from triaxial orbit-superposition Schwarzschild models

Giulia Santucci, Sarah Brough, Jesse van de Sande +17

Dynamical models are crucial for uncovering the internal dynamics of galaxies, however, most of the results to date assume axisymmetry, which is not representative for a significan…

astro-ph.GA2022★ 24 cited

The SAMI Galaxy Survey: the difference between ionised gas and stellar velocity dispersions

Sree Oh, Matthew Colless, Francesco D'Eugenio +16

We investigate the mean locally-measured velocity dispersions of ionised gas () and stars () for 1090 galaxies with stellar masses $\log\,(M_*/M_{\odot}) \geq 9.5…