249 citations · 733 across the 20 of their papers we have counts for
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Deep Extragalactic VIsible Legacy Survey (DEVILS): Identification of AGN through SED Fitting and the Evolution of the Bolometric AGN Luminosity Function
Jessica E. Thorne, Aaron S. G. Robotham, Luke J. M. Davies +15
Active galactic nuclei (AGN) are typically identified through radio, mid-infrared, or X-ray emission or through the presence of broad and/or narrow emission lines. AGN can also lea…
Deep Extragalactic VIsible Legacy Survey (DEVILS): Evolution of the -M relation and implications for self-regulated star formation
L. J. M. Davies, J. E. Thorne, S. Bellstedt +13
We present the evolution of the star-formation dispersion - stellar mass relation (-M) in the DEVILS D10 region using new measurements derived using the ProSpect…
Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
Matías Bravo, Eric Gawiser, Nelson D. Padilla +3
The high cosmological precision offered by the next generation of galaxy surveys hinges on improved corrections for Galactic dust extinction. We explore the possibility of estimati…
Deep Extragalactic VIsible Legacy Survey (DEVILS): Consistent multi-wavelength photometry for the DEVILS regions (COSMOS, XMMLSS & ECDFS)
L. J. M. Davies, J. E. Thorne, A. S. G. Robotham +23
The Deep Extragalactic VIsible Legacy Survey (DEVILS) is an ongoing high-completeness, deep spectroscopic survey of 60,000 galaxies to Y21.2 mag, over 6 deg2 in thre…
Forensic reconstruction of galaxy colour evolution and population characterisation
Matías Bravo, Aaron S. G. Robotham, Claudia del P. Lagos +3
Mapping the evolution of galaxy colours, from blue star-forming to red passive systems, is fundamental to understand the processes involved in galaxy evolution. To this end, we rec…
Unveiling the atomic hydrogen-halo mass relation via spectral stacking
Garima Chauhan, Claudia del P. Lagos, Adam R. H. Stevens +5
Measuring the HI-halo mass scaling relation (HIHM) is fundamental to understanding the role of HI in galaxy formation and its connection to structure formation. While direct measur…