activity
20112025
most citedGalaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV --- far-IR) and the low-z energy budget

166 citations · 474 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2025★ 3 cited

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.GA2018★ 95 cited

The SAMI Galaxy Survey: Data Release Two with absorption-line physics value-added products

Nicholas Scott, Jesse van de Sande, Scott M. Croom +34

We present the second major release of data from the SAMI Galaxy Survey. Data Release Two includes data for 1559 galaxies, about 50% of the full survey. Galaxies included have a re…

astro-ph.GA2018★ 114 cited

Deep Extragalactic VIsible Legacy Survey (DEVILS): Motivation, Design and Target Catalogue

L. J. M. Davies, A. S. G. Robotham, S. P. Driver +26

The Deep Extragalactic VIsible Legacy Survey (DEVILS) is a large spectroscopic campaign at the Anglo-Australian Telescope (AAT) aimed at bridging the near and distant Universe by p…

astro-ph.GA2017★ 78 cited

The SAMI Galaxy Survey: Data Release One with Emission-line Physics Value-Added Products

Andrew W. Green, Scott M. Croom, Nicholas Scott +48

We present the first major release of data from the SAMI Galaxy Survey. This data release focuses on the emission-line physics of galaxies. Data Release One includes data for 772 g…

astro-ph.GA2015★ 166 cited

Galaxy And Mass Assembly (GAMA): Panchromatic Data Release (far-UV --- far-IR) and the low-z energy budget

Simon P. Driver, Angus H. Wright, Stephen K. Andrews +60

We present the GAMA Panchromatic Data Release (PDR) constituting over 230deg of imaging with photometry in 21 bands extending from the far-UV to the far-IR. These data compleme…

astro-ph.CO2013★ 4 cited

Identifying clustering at high redshift through actively star-forming galaxies

L. J. M. Davies, M. N. Bremer, E. R. Stanway +3

Identifying galaxy clustering at high redshift (i.e. z > 1) is essential to our understanding of the current cosmological model. However, at increasing redshift, clusters evolve co…