Deep Extragalactic VIsible Legacy Survey (DEVILS): Motivation, design, and target catalogue

Authors

L. J.M. Davies, The University of Western Australia
A. S.G. Robotham, The University of Western Australia
S. P. Driver, The University of Western Australia
C. P. Lagos, The University of Western Australia
L. Cortese, The University of Western Australia
E. Mannering, The University of Western Australia
C. Foster, The University of Sydney
C. Lidman, The Australian National University
A. Hashemizadeh, The University of Western Australia
S. Koushan, The University of Western Australia
S. O'Toole, Australian Astronomical Observatory
I. K. Baldry, Liverpool John Moores University
M. Bilicki, Leiden Observatory Research Institute
J. Bland-Hawthorn, The University of Sydney
M. N. Bremer, University of Bristol
M. J.I. Brown, Monash University
J. J. Bryant, Australian Astronomical Observatory
B. Catinella, The University of Western Australia
S. M. Croom, The University of Sydney
M. W. Grootes, ESA/ESTEC SCI-S
Benne W. Holwerda, University of LouisvilleFollow
M. J. Jarvis, University of Oxford
N. Maddox, Netherlands Foundation for Research in Astronomy
M. Meyer, The University of Western Australia
A. J. Moffett, Vanderbilt University
S. Phillipps, University of Bristol
E. N. Taylor, Swinburne University of Technology
R. A. Windhorst, School of Earth and Space Exploration
C. Wolf, The Australian National University

Document Type

Article

Publication Date

10-11-2018

Department

Physics and Astronomy

Abstract

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 producing the highest completeness survey of galaxies and groups at intermediate redshifts (0.3 < z < 1.0). Our sample consists of ~60 000 galaxies to Y < 21.2mag, over ~6 deg2 in threewell-studied deep extragalactic fields (Cosmic Origins Survey field, COSMOS; Extended Chandra Deep Field South, ECDFS; and the X-ray Multi-Mirror Mission Large-Scale Structure region, XMM-LSS - all Large Synoptic Survey Telescope deep-drill fields). This paper presents the broad experimental design of DEVILS. Our target sample has been selected from deep Visible and Infrared Survey Telescope for Astronomy (VISTA) Y-band imaging (VISTA Deep Extragalactic Observations, VIDEO and UltraVISTA), with photometry measured by PROFOUND. Photometric star/galaxy separation is done on the basis of near-infrared colours and has been validated by visual inspection. To maximize our observing efficiency for faint targets, we employ a redshift feedback strategy, which continually updates our target lists, feeding back the results from the previous night's observations. We also present an overview of the initial spectroscopic observations undertaken in late 2017 and early 2018.

ThinkIR Citation

Davies, L. J.M.; Robotham, A. S.G.; Driver, S. P.; Lagos, C. P.; Cortese, L.; Mannering, E.; Foster, C.; Lidman, C.; Hashemizadeh, A.; Koushan, S.; O'Toole, S.; Baldry, I. K.; Bilicki, M.; Bland-Hawthorn, J.; Bremer, M. N.; Brown, M. J.I.; Bryant, J. J.; Catinella, B.; Croom, S. M.; Grootes, M. W.; Holwerda, Benne W.; Jarvis, M. J.; Maddox, N.; Meyer, M.; Moffett, A. J.; Phillipps, S.; Taylor, E. N.; Windhorst, R. A.; and Wolf, C., "Deep Extragalactic VIsible Legacy Survey (DEVILS): Motivation, design, and target catalogue" (2018). Faculty and Staff Scholarship. 497.
https://ir.library.louisville.edu/faculty/497

DOI

10.1093/mnras/sty1553

ORCID

0000-0002-4884-6756