Journal article
Extragalactic Peaked-spectrum Radio Sources at Low Frequencies
JR Callingham, RD Ekers, BM Gaensler, JLB Line, N Hurley-Walker, EM Sadler, SJ Tingay, PJ Hancock, ME Bell, KS Dwarakanath, B-Q For, TMO Franzen, L Hindson, M Johnston-Hollitt, AD Kapinska, E Lenc, B McKinley, J Morgan, AR Offringa, P Procopio Show all
The Astrophysical Journal | IOP PUBLISHING LTD | Published : 2017
Grants
Awarded by Australian Research Council Centre of Excellence for Allsky Astrophysics (CAASTRO)
Awarded by Natural Sciences and Engineering Research Council of Canada (NSERC)
Awarded by Science and Technology Facilities Council
Funding Acknowledgements
This scientific work makes use of the Murchison Radioastronomy Observatory, operated by CSIRO. We acknowledge the Wajarri Yamatji people as the traditional owners of the Observatory site. Support for the operation of the MWA is provided by the Australian Government (NCRIS), under a contract to Curtin University administered by Astronomy Australia Limited. We acknowledge the Pawsey Supercomputing Centre, which is supported by the Western Australian and Australian Governments. This research was conducted by the Australian Research Council Centre of Excellence for Allsky Astrophysics (CAASTRO), through project number CE110001020. J.R.C. acknowledges the support of the Australian Postgraduate Award. The Dunlap Institute is funded through an endowment established by the David Dunlap family and the University of Toronto. B.M.G. acknowledges the support of the Natural Sciences and Engineering Research Council of Canada (NSERC) through grant RGPIN-2015-05948, and of the Canada Research Chairs program. 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, and the VizieR catalog access tool, CDS, Strasbourg, France. Topcat (Taylor 2005), SAOImage DS9, NASA's Astrophysics Data System bibliographic services, and Astropy, a community-developed core Python package for Astronomy (Astropy Collaboration et al. 2013), were also used in this study.