collaborators

6 papers

astro-ph.GA2025

Deep Extragalactic VIsible Legacy Survey (DEVILS): First Data Release Covering The D10 (COSMOS) Region

L. J. M. Davies, M. Bravo, R. H. W. Cook +18

The Deep Extragalactic VIsible Legacy Survey (DEVILS) is a deep, high-completeness multi-wavelength survey based around spectroscopic observations using the Anglo-Australian Telesc…

astro-ph.GA2025

Deep Extragalactic VIsible Legacy Survey (DEVILS): Evolution of the Morphology-Density Relation

L. J. M. Davies, J. Doan, S. Bellstedt +6

Galaxies with different morphological characteristics likely have different evolutionary histories, such that understanding the mechanisms that drive morphological change can provi…

astro-ph.GA2025

Deep Extragalactic VIsible Legacy Survey (DEVILS): Satellite Quenching at Intermediate Redshift

L. J. M. Davies, M. F. Fuentealba-Fuentes, R. J. Wright +3

Determining the processes by which galaxies transition from a star-forming to a quiescent state (quenching) is paramount to our understanding of galaxy evolution. One of the key me…

astro-ph.GA2025

Correcting for the effects of the point spread function in intra-halo light measurements and application to deep Hyper Suprime-Cam data

L. P. Garate-Nuñez, A. S. G. Robotham, S. Bellstedt +1

The intra-halo light (IHL) is the diffuse stellar component that surrounds galaxies, groups, and clusters. Its formation is intimately linked to the hierarchical assembly of the sy…

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)…