4.4 Article

The Murchison Widefield Array Commissioning Survey: A Low-Frequency Catalogue of 14 110 Compact Radio Sources over 6 100 Square Degrees

Publisher

CAMBRIDGE UNIV PRESS
DOI: 10.1017/pasa.2014.40

Keywords

radio continuum: general; surveys; techniques: interferometric

Funding

  1. U.S. National Science Foundation [AST-0457585, PHY-0835713, CAREER-0847753, AST-0908884]
  2. Australian Research Council (LIEF grants) [LE0775621, LE0882938]
  3. U.S. Air Force Office of Scientific Research [FA9550-0510247]
  4. Centre for All-sky Astrophysics (an Australian Research Council Centre of Excellence) [CE110001020]
  5. Smithsonian Astrophysical Observatory
  6. MIT School of Science
  7. Raman Research Institute
  8. Australian National University
  9. Victoria University of Wellington (New Zealand Ministry of Economic Development and an IBM Shared University Research Grant)
  10. Commonwealth Scientific and Industrial Research Organisation (CSIRO)
  11. National Collaborative Research Infrastructure Strategy
  12. Education Investment Fund
  13. Australia India Strategic Research Fund
  14. Astronomy Australia Limited
  15. Western Australian State government
  16. [MED-E1799]

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We present the results of an approximately 6 100 deg(2) 104-196 MHz radio sky survey performed with the Murchison Widefield Array during instrument commissioning between 2012 September and 2012 December: the MWACS. The data were taken as meridian drift scans with two different 32-antenna sub-arrays that were available during the commissioning period. The survey covers approximately 20.5 h< RA < 8.5 h, -58 degrees < Dec < -14 degrees over three frequency bands centred on 119, 150 and 180 MHz, with image resolutions of 6-3 arcmin. The catalogue has 3 arcmin angular resolution and a typical noise level of 40 mJy beam(-1), with reduced sensitivity near the field boundaries and bright sources. We describe the data reduction strategy, based upon mosaicked snapshots, flux density calibration, and source-finding method. We present a catalogue of flux density and spectral index measurements for 14 110 sources, extracted from the mosaic, 1 247 of which are sub-components of complexes of sources.

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