activity
20162026
most cited4MOST: Project overview and information for the First Call for Proposals

311 citations · 2.3k across the 89 of their papers we have counts for

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Showing 2021Show all

10 papers · 1 filter

astro-ph.GA2021★ 53 cited

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…

astro-ph.GA2021★ 16 cited

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…

astro-ph.GA2021★ 3 cited

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…

astro-ph.GA2021★ 5 cited

Galaxy And Mass Assembly (GAMA): Galaxy Luminosity Function down to via Clustering Based Redshift Inference

Geray S. Karademir, Edward N. Taylor, Chris Blake +12

In this study we present a new experimental design using clustering-based redshift inference to measure the evolving galaxy luminosity function (GLF) spanning 5.5 decades from $L \…

astro-ph.GA2021★ 46 cited

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…

astro-ph.GA2021★ 17 cited

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…

astro-ph.GA2021★ 45 cited

Galaxy And Mass Assembly (GAMA): The inferred mass--metallicity relation from z=0 to 3.5 via forensic SED fitting

Sabine Bellstedt, Aaron S. G. Robotham, Simon P. Driver +7

We analyse the metallicity histories of ~4,500 galaxies from the GAMA survey at z<0.06 modelled by the SED-fitting code ProSpect using an evolving metallicity implementation. These…

astro-ph.GA2021★ 15 cited

Deep Extragalactic VIsible Legacy Survey (DEVILS): Stellar Mass Growth by Morphological Type since

Abdolhosein Hashemizadeh, Simon P. Driver, Luke J. M. Davies +13

Using high-resolution Hubble Space Telescope imaging data, we perform a visual morphological classification of galaxies at in the DEVILS/COSMOS region. As the…

astro-ph.CO2021★ 45 cited

GAMA/DEVILS: Constraining the cosmic star-formation history from improved measurements of the 0.3-2.2 micron Extragalactic Background Light

Soheil Koushan, Simon P. Driver, Sabine Bellstedt +12

We present a revised measurement of the optical extragalactic background light (EBL), based on the contribution of resolved galaxies to the integrated galaxy light (IGL). The cosmi…

astro-ph.GA2021★ 31 cited

Remnant Radio Galaxies Discovered in a Multi-frequency Survey

B. Quici, N. Hurley-Walker, N. Seymour +20

The remnant phase of a radio galaxy begins when the jets launched from an active galactic nucleus are switched off. To study the fraction of radio galaxies in a remnant phase, we t…