collaborators

10 papers

astro-ph.GA2026

Kinematic scaling of thin and thick discs from SAMI to NewHorizon

Sree Oh, J. K. Jang, Giulia Santucci +8

We revisit the relation between disc stellar mass and disc velocity dispersion (M_*-σ_e) and extend it to thin and thick subcomponents using orbit-based dynamical models of 161 SA…

astro-ph.GA2026

Morphology-spin connection in the SAMI Galaxy Survey

Youngmin Baek, Sree Oh, Sukyoung K. Yi +5

The spin parameter is a proxy for the specific stellar angular momentum of galaxies and is a useful metric for classifying kinematic morphology. This study aims to…

astro-ph.IM2026

WST -- Wide-field Spectroscopic Telescope: The Next Leap in Wide-field Spectroscopy

Roland Bacon, Olga Bellido, Philippe Dierickx +53

The Wide-field Spectroscopic Telescope (WST) is a concept for a dedicated 12-m spectroscopic survey facility designed to address some of the most important questions in astrophysic…

astro-ph.GA2026

Hector Galaxy Survey: Linking the low- and high-mass ends of the initial mass function in star-forming galaxies

Diego Salvador, Andrew Hopkins, Matt Owers +30

The stellar initial mass function (IMF) is a fundamental ingredient in galaxy evolution, linking observed integrated light to galaxy properties. Constraining the full IMF shape bey…

astro-ph.GA2026

Large-scale and local environmental drivers of quenching: tracing H concentration in X-ray and optical galaxy groups

Stefania Barsanti, Di Wang, Matthew Colless +11

To explore the environmental mechanisms causing quenching in nearby star-forming galaxies, we study the variation with local and large-scale environments of a star formation concen…

astro-ph.GA2025

Spin-filament alignments to unravel galaxy evolution and model intrinsic alignments

Stefania Barsanti, Clotilde Laigle, Nicolas Bouché +7

By the 2040s, several all-sky surveys will have transformed our view of the large-scale structure. However, one of the major outstanding questions in astrophysics will remain: unde…