570 citations · 3.7k across the 31 of their papers we have counts for
31 papers
Ageing and Quenching through the ageing diagram II: physical characterization of galaxies
Pablo Corcho-Caballero, Yago Ascasibar, Luca Cortese +4
The connection between quenching mechanisms, which rapidly turn star-forming systems into quiescent, and the properties of the galaxy population remains difficult to discern. In th…
GRB 180325A: dust grain-size distribution and interstellar iron nanoparticles contribution
Elizabeth Cappellazzo, Tayyaba Zafar, Pablo Corcho-Caballero +3
We modelled dust grain-size distributions for carbonaceous and silicates dust, as well as for free-flying iron nanoparticles in the environment of a -ray burst (GRB) afterglow,…
The SAMI Galaxy Survey: First detection of a transition in spin orientation with respect to cosmic filaments in the stellar kinematics of galaxies
C. Welker, J. Bland-Hawthorn, J. Van de Sande +16
We present the first detection of mass dependent galactic spin alignments with local cosmic filaments with over 2 sigma confidence using IFS kinematics. The 3D network of cosmic fi…
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…
The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations
E. Tescari, L. Cortese, C. Power +23
This work presents a study of galactic outflows driven by stellar feedback. We extract main sequence disc galaxies with stellar mass MM$_{\odot} \le 5.7\times1…
The SAMI Galaxy Survey: mass as the driver of the kinematic morphology - density relation in clusters
Sarah Brough, Jesse van de Sande, Matt S. Owers +23
We examine the kinematic morphology of early-type galaxies (ETGs) in eight galaxy clusters in the Sydney-AAO Multi-object Integral field spectrograph (SAMI) Galaxy Survey. The clus…