A Large-Scale, Low-Frequency Murchison Widefield Array Survey of Galactic H II Regions between 260 < l < 340

L Hindson; M Johnston-Hollitt; N Hurley-Walker; JR Callingham; H Su; J Morgan; M Bell; G Bernardi; JD Bowman; F Briggs; RJ Cappallo; AA Deshpande; KS Dwarakanath; B-Q For; BM Gaensler; LJ Greenhill; P Hancock; BJ Hazelton; AD Kapinska; DL Kaplan; E Lenc; CJ Lonsdale; B Mckinley; SR McWhirter; DA Mitchell; MF Morales; E Morgan; D Oberoi; A Offringa; SM Ord; P Procopio; T Prabu; N Udaya Shankar; KS Srivani; L Staveley-Smith; R Subrahmanyan; SJ Tingay; RB Wayth; RL Webster; A Williams; CL Williams; C Wu; Q Zheng

Journal article

A Large-Scale, Low-Frequency Murchison Widefield Array Survey of Galactic H II Regions between 260 < l < 340

L Hindson, M Johnston-Hollitt, N Hurley-Walker, JR Callingham, H Su, J Morgan, M Bell, G Bernardi, JD Bowman, F Briggs, RJ Cappallo, AA Deshpande, KS Dwarakanath, B-Q For, BM Gaensler, LJ Greenhill, P Hancock, BJ Hazelton, AD Kapinska, DL Kaplan Show all

Publications of the Astronomical Society of Australia | CAMBRIDGE UNIV PRESS | Published : 2016

DOI: 10.1017/pasa.2016.19

University of Melbourne Researchers

Pietro Procopio Author Melbourne School of Population and Global Health

Grants

Awarded by Ministry of Business, Employment AMP; Innovation, New Zealand

Funding Acknowledgements

LH was partially supported in this work via grant MED E1799 (PI: Johnston-Hollitt) provided by the Ministry of Business, Employment & Innovation, New Zealand. MJ-H acknowledges support from the Marsden Fund. This scientific work makes use of the Murchison Radio-astronomy Observatory, operated by CSIRO. We acknowledge the Wajarri Yamatji people as the traditional owners of the Observatory site. We acknowledge the iVEC Petabyte Data Store, the Initiative in Innovative Computing and the CUDA Center for Excellence sponsored by NVIDIA at Harvard University. The authors thank the referee for their very useful comments that resulted in the improvement of this paper.