465 citations · 2k across the 125 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…
Deep Extragalactic VIsible Legacy Survey (DEVILS): DR1 Blended Spectra Search for Candidate Strong Gravitational Lenses
B. W. Holwerda, S. Knabel, J. E Thorne +3
Here, we present a catalog of blended spectra in Data Release 1 of the Deep Extragalactic VIsible Legacy Survey (DEVILS) on the Anglo-Australian Telescope (AAT). Of the 23197 spect…
The Type II AGN-host galaxy connection: insights from the VVDS and VIPERS surveys
G. Vietri, B. Garilli, M. Polletta +16
We present a study of optically-selected Type II AGN at 0.5 < z < 0.9 from the VIPERS and VVDS surveys, to investigate the connection between AGN activity and physical properties o…
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…
The PAU Survey: Measurement of Narrow-band galaxy properties with Approximate Bayesian Computation
Luca Tortorelli, Malgorzata Siudek, Beatrice Moser +22
Narrow-band imaging surveys allow the study of the spectral characteristics of galaxies without the need of performing their spectroscopic follow-up. In this work, we forward-model…