activity
20242026
collaborators
Showing 2025Show all

9 papers · 1 filter

astro-ph.GA2025

Galaxy Mergers in the Epoch of Reionization I: A JWST Study of Pair Fractions, Merger Rates, and Stellar Mass Accretion Rates at

Qiao Duan, Christopher J. Conselice, Qiong Li +30

We present a full analysis of galaxy major merger pair fractions, merger rates, and mass accretion rates, thus uncovering the role of mergers in galaxy formation at the earliest pr…

astro-ph.GA2025

Deep Extragalactic VIsible Legacy Survey (DEVILS): The sSFR-M plane part II: Starbursts, SFHs and AGN Feedback

L. J. M. Davies, J. E. Thorne, S. Bellstedt +10

In part I of this series we discussed the variation of star-formation histories (SFHs) across the specific star formation rate - stellar mass plane (sSFR-M) using the Dee…

astro-ph.GA2025

Deep Extragalactic VIsible Legacy Survey (DEVILS): The sSFR-Mplane part I: The recent SFH of galaxies and movement through the plane

L. J. M. Davies, J. E. Thorne, S. Bellstedt +10

In a recent paper we parameterised the evolution of the star-formation rate dispersion () across the specific star-formation rate - stellar mass plane (sSFR-M)…

astro-ph.GA2025

WALLABY pilot survey: Spatially resolved gas scaling relations within the stellar discs of nearby galaxies

Seona Lee, Barbara Catinella, Tobias Westmeier +13

The scatter in global atomic hydrogen (HI) scaling relations is partly attributed to differences in how HI and stellar properties are measured, with HI reservoirs typically extendi…

astro-ph.GA2025

Galaxy And Mass Assembly: A new approach to quantifying dust in galaxies

B. Farley, U. T. Ahmed, A. M. Hopkins +8

We introduce a new approach to quantifying dust in galaxies by combining information from the Balmer decrement (BD) and the dust mass (). While there is no explicit correlatio…

astro-ph.GA2025

A comparison of dust content and properties in GAMA/G10-COSMOS/3D-HST and SIMBA cosmological simulations

Trevor Butrum, Benne Holwerda, Romeel Dave +3

The abundance of dust within galaxies directly influences their evolution. Contemporary models attempt to match this abundance by simulating the processes of dust creation, growth,…