Journal article

Wide-field broad-band radio imaging with phased array feeds: a pilot multi-epoch continuum survey with ASKAP-BETA

I Heywood, KW Bannister, J Marvil, JR Allison, L Ball, ME Bell, DC-J Bock, M Brothers, JD Bunton, AP Chippendale, F Cooray, TJ Cornwell, D De Boer, P Edwards, R Gough, N Gupta, L Harvey-Smith, S Hay, AW Hotan, B Indermuehle Show all

Monthly Notices of the Royal Astronomical Society | OXFORD UNIV PRESS | Published : 2016

University of Melbourne Researchers

Grants

Awarded by Australian Research Council Centre of Excellence for All-sky Astrophysics (CAAS-TRO)


Awarded by National Science Foundation


Awarded by National Aeronautics and Space Administration's Earth Science Technology Office, Computation Technologies Project


Funding Acknowledgements

We thank the anonymous referee and the MNRAS editorial staff for their comments on this paper. The Australian SKA Pathfinder is part of the Australia Telescope National Facility which is managed by CSIRO. Operation of ASKAP is funded by the Australian Government with support from the National Collaborative Research Infrastructure Strategy. Establishment of the Murchison Radio-astronomy Observatory was funded by the Australian Government and the Government of Western Australia. ASKAP uses advanced supercomputing resources at the Pawsey Supercomputing Centre. We acknowledge the Wajarri Yamatji people as the traditional owners of the Observatory site. This work was supported by resources provided by the Pawsey Supercomputing Centre with funding from the Australian Government and the Government of Western Australia. Parts of this research were conducted by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAAS-TRO), through project number CE110001020. This research made use of Montage. It is funded by the National Science Foundation under Grant Number ACI-1440620, and was previously funded by the National Aeronautics and Space Administration's Earth Science Technology Office, Computation Technologies Project, under Co-operative Agreement Number NCC5-626 between NASA and the California Institute of Technology. This research has made use of NASA's Astrophysics Data System. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. IH acknowledges many useful discussions with Jan Noordam, Rick Perley and Oleg Smirnov.