John H.Y. Ching
The Large Area Radio Galaxy Evolution Spectroscopic Survey (LARGESS): survey design, data catalogue and GAMA/WiggleZ spectroscopy
Ching, John H.Y.; Sadler, Elaine M.; Croom, Scott M.; Johnston, Helen M.; Pracy, Michael B.; Couch, Warrick J.; Hopkins, A. M.; Jurek, Russell J.; Pimbblet, K. A.
Authors
Elaine M. Sadler
Scott M. Croom
Helen M. Johnston
Michael B. Pracy
Warrick J. Couch
A. M. Hopkins
Russell J. Jurek
Dr Kevin Pimbblet K.Pimbblet@hull.ac.uk
Director of DAIM
Abstract
© 2016 The Authors. We present the Large Area Radio Galaxy Evolution Spectroscopic Survey (LARGESS), a spectroscopic catalogue of radio sources designed to include the full range of radio AGN populations out to redshift z ~ 0.8. The catalogue covers ~800 deg 2 of sky, and provides optical identifications for 19 179 radio sources from the 1.4 GHz Faint Images of the Radio Sky at Twenty-cm (FIRST) survey down to an optical magnitude limit of i mod < 20.5 in Sloan Digital Sky Survey (SDSS) images. Both galaxies and point-like objects are included, and no colour cuts are applied. In collaboration with the WiggleZ and Galaxy And Mass Assembly (GAMA) spectroscopic survey teams, we have obtained new spectra for over 5000 objects in the LARGESS sample. Combining these new spectra with data from earlier surveys provides spectroscopic data for 12 329 radio sources in the survey area, of which 10 856 have reliable redshifts. 85 per cent of the LARGESS spectroscopic sample are radio AGN (median redshift z = 0.44), and 15 per cent are nearby star-forming galaxies (median z = 0.08). Low-excitation radio galaxies (LERGs) comprise the majority (83 per cent) of LARGESS radio AGN at z < 0.8, with 12 per cent being high-excitation radio galaxies (HERGs) and 5 per cent radioloud QSOs. Unlike the more homogeneous LERG and QSO sub-populations, HERGs are a heterogeneous class of objects with relatively blue optical colours and a wide dispersion in mid-infrared colours. This is consistent with a picture in which most HERGs are hosted by galaxies with recent or ongoing star formation as well as a classical accretion disc.
Citation
Ching, J. H., Sadler, E. M., Croom, S. M., Johnston, H. M., Pracy, M. B., Couch, W. J., …Pimbblet, K. A. (2017). The Large Area Radio Galaxy Evolution Spectroscopic Survey (LARGESS): survey design, data catalogue and GAMA/WiggleZ spectroscopy. Monthly notices of the Royal Astronomical Society, 464(2), 1306-1332. https://doi.org/10.1093/mnras/stw2396
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 20, 2016 |
Online Publication Date | Sep 21, 2016 |
Publication Date | Jan 11, 2017 |
Deposit Date | Sep 23, 2016 |
Publicly Available Date | Sep 23, 2016 |
Journal | Monthly notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 464 |
Issue | 2 |
Pages | 1306-1332 |
DOI | https://doi.org/10.1093/mnras/stw2396 |
Keywords | Radio continuum -- galaxies, Galaxies -- active, Catalogues, Surveys |
Public URL | https://hull-repository.worktribe.com/output/443504 |
Publisher URL | http://mnras.oxfordjournals.org/content/early/2016/09/21/mnras.stw2396.abstract |
Additional Information | This article has been accepted for publication in Monthly notices of the Royal Astronomical Society ©: 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. |
Files
Article.pdf
(9.9 Mb)
PDF
Copyright Statement
© 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society
You might also like
How typical is the Coma cluster?
(2014)
Journal Article
Photometric studies of Abell 1664: the subtle effect a minor merger has on cluster galaxies
(2014)
Journal Article
Galaxy and Mass Assembly (GAMA) : fine filaments of galaxies detected within voids
(2014)
Journal Article
Distribution of slow and fast rotators in the Fornax cluster
(2014)
Journal Article