collaborators
Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2025

GAMA 526784: the progenitor of a globular cluster-rich ultra-diffuse galaxy? I. Star clusters, stellar body and ionised gas properties

Maria Luisa Buzzo, Michael Hilker, Anita Zanella +4

Context. Ultra-diffuse galaxies (UDGs) are an intriguing population of galaxies. Despite their dwarf-like stellar masses and low surface brightness, they have large half-light radi…

astro-ph.GA2024

Pulling back the curtain on shocks and star-formation in NGC 1266 with Gemini-NIFS

Justin Atsushi Otter, Katherine Alatalo, Kate Rowlands +21

We present Gemini near-infrared integral field spectrograph (NIFS) K-band observations of the central 400 pc of NGC 1266, a nearby (D30 Mpc) post-starburst galaxy with a p…

astro-ph.GA2024

The MAGPI Survey: Orbital distributions, intrinsic shapes, and mass profiles for MAGPI-like Eagle galaxies using Schwarzschild dynamical models

Giulia Santucci, Claudia Del P. Lagos, Katherine E. Harborne +16

Schwarzschild dynamical models are now regularly employed in large surveys of galaxies in the local and distant Universe to derive information on galaxies' intrinsic properties suc…

astro-ph.GA2024

The MAGPI Survey: Massive slow rotator population in place by

Caro Derkenne, Richard M. McDermid, Francesco D'Eugenio +20

We use the `Middle Ages Galaxy Properties with Integral field spectroscopy' (MAGPI) survey to investigate whether galaxies have evolved in the distribution of their stellar angular…

astro-ph.GA2024

The SAMI galaxy survey: predicting kinematic morphology with logistic regression

Sam P. Vaughan, Jesse van de Sande, A. Fraser-McKelvie +10

We use the SAMI galaxy survey to study the the kinematic morphology-density relation: the observation that the fraction of slow rotator galaxies increases towards dense environment…