Repository logo
  • English
  • Italiano
Log In
Have you forgotten your password?
  1. Home
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
  5. LOFAR/H-ATLAS: a deep low-frequency survey of the Herschel-ATLAS North Galactic Pole field
 

LOFAR/H-ATLAS: a deep low-frequency survey of the Herschel-ATLAS North Galactic Pole field

Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY  
Date Issued
2016
Author(s)
Hardcastle, M. J.
•
Gürkan, G.
•
van Weeren, R. J.
•
Williams, W. L.
•
Best, P. N.
•
De Gasperin, F.  
•
Rafferty, D. A.
•
READ, SHAUN CONISBEE  
•
Sabater, J.
•
Shimwell, T. W.
•
Smith, D. J. B.
•
Tasse, C.
•
Bourne, N.
•
BRIENZA, MARISA  
•
Brüggen, M.
•
BRUNETTI, GIANFRANCO  
•
Chyży, K. T.
•
Conway, J.
•
Dunne, L.
•
Eales, S. A.
•
Maddox, S. J.
•
Jarvis, M. J.
•
Mahony, E. K.
•
Morganti, R.
•
PRANDONI, ISABELLA  
•
Röttgering, H. J. A.
•
Valiante, E.
•
White, G. J.
DOI
10.1093/mnras/stw1763
Abstract
We present Low-Frequency Array (LOFAR) High-Band Array observations of the Herschel-ATLAS North Galactic Pole survey area. The survey we have carried out, consisting of four pointings covering around 142 deg2 of sky in the frequency range 126-173 MHz, does not provide uniform noise coverage but otherwise is representative of the quality of data to be expected in the planned LOFAR wide-area surveys, and has been reduced using recently developed `facet calibration' methods at a resolution approaching the full resolution of the data sets (∼10 × 6 arcsec) and an rms off-source noise that ranges from 100 μJy beam-1 in the centre of the best fields to around 2 mJy beam-1 at the furthest extent of our imaging. We describe the imaging, cataloguing and source identification processes, and present some initial science results based on a 5σ source catalogue. These include (I) an initial look at the radio/far-infrared correlation at 150 MHz, showing that many Herschel sources are not yet detected by LOFAR; (II) number counts at 150 MHz, including, for the first time, observational constraints on the numbers of star-forming galaxies; (III) the 150-MHz luminosity functions for active and star-forming galaxies, which agree well with determinations at higher frequencies at low redshift, and show strong redshift evolution of the star-forming population; and (IV) some discussion of the implications of our observations for studies of radio galaxy life cycles.
Volume
462
Issue
2
Start page
1910
Uri
http://hdl.handle.net/20.500.12386/24318
Url
https://academic.oup.com/mnras/article/462/2/1910/2589854
http://arxiv.org/abs/1606.09437v1
Issn Identifier
0035-8711
Ads BibCode
2016MNRAS.462.1910H
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

1606.09437.pdf

Description
postprint
Size

13.94 MB

Format

Adobe PDF

Checksum (MD5)

5f0cdb1eb2bd2cac6d37db0e3567ed1f

Loading...
Thumbnail Image
Name

stw1763_compressed.pdf

Description
pdf editoriale
Size

9.43 MB

Format

Adobe PDF

Checksum (MD5)

193774c2ca9f68cc69065fa0411659e6

Explore By
  • Communities and Collection
  • Research Outputs
  • Researchers
  • Organizations
  • Projects
Information and guides for authors
  • https://openaccess-info.inaf.it: all about open access in INAF
  • How to enter a product: guides to OA@INAF
  • The INAF Policy on Open Access
  • Downloadable documents and templates

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback