collaborators

6 papers

astro-ph.GA2025

Super-resolving Herschel - a deep learning based deconvolution and denoising technique

Dennis Koopmans, Lingyu Wang, Berta Margalef-Bentabol +9

Dusty star-forming galaxies (DSFGs) dominate the far-infrared and sub-millimetre number counts, but single-dish surveys suffer from poor angular resolution, complicating mult-wavel…

astro-ph.CO2025

Wide Area VISTA Extragalactic Survey (WAVES): Selection of targets for the Wide survey using decision-tree classification

G. Kaur, M. Bilicki, S. Bellstedt +11

The Wide-Area VISTA Extragalactic Survey (WAVES) on the 4-metre Multi-Object Spectroscopic Telescope (4MOST) includes two flux-limited subsurveys with very high (95\%) completeness…

astro-ph.GA2025

Nessie: A Rust-Powered, Fast, Flexible, and Generalized Friends-of-Friends Galaxy-Group Finder in R and Python

Trystan S. Lambert, A. S. G. Robotham, M. Bravo +4

We introduce Nessie, a galaxy group finder implemented in Rust and distributed as both a Python and R package. Nessie employs the friends-of-friends (FoF) algorithm and requires on…

astro-ph.GA2025

Deep Extragalactic VIsible Legacy Survey (DEVILS): Galaxy group catalogue for the D10-COSMOS field with 90% spectroscopic redshift completeness

Matías Bravo, Luke J. M. Davies, Aaron S. G. Robotham +6

Large-scale galaxy redshift surveys conducted over the last couple of decades have proven crucial in deepening our understanding of structure growth in the Universe and galaxy evol…

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)…