51. Australian Square Kilometre Array Pathfinder: I. System Description
- Author
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John D. Bunton, S. Johnston, J. Tuthill, Douglas C.-J. Bock, Aaron Chippendale, Wasim Raja, Grant Hampson, Anastasios Tzioumis, Aidan Hotan, James R. Allison, Ron Beresford, R. McConigley, David McConnell, Emil Lenc, E. R. Troup, K. Chow, Paolo Serra, Jessica M. Chapman, S. W. Amy, T. Sweetnam, Douglas B. Hayman, Matthew Whiting, R. Bolton, M. A. Pilawa, E. Bastholm, E. S. Lensson, Vanessa A. Moss, C. A. Jackson, C. Jacka, Thomas M. O. Franzen, Keith W. Bannister, Tobias Westmeier, D. George, Sarah Pearce, Elizabeth K. Mahony, Maxim Voronkov, Elaine M. Sadler, A. Ng, Daniel N. Roxby, I. Heywood, Lisa Harvey-Smith, Ilana Feain, D. Kleiner, John Reynolds, S. Mackay, Tim J. Cornwell, Ray P. Norris, Robert D. Shaw, A. E. T. Schinckel, M. Shields, Paul Roberts, Neeraj Gupta, F. R. Cooray, Chris Phillips, Naomi McClure-Griffiths, Michael Kesteven, M. T. Huynh, Craig S. Anderson, Jordan D. Collier, Philip G. Edwards, Philip J. Diamond, P. Mirtschin, K. Jeganathan, Baerbel Koribalski, K. Lee-Waddell, and S. Jackson
- Subjects
Physics ,Phased array feed ,business.industry ,Astrophysics::Instrumentation and Methods for Astrophysics ,FOS: Physical sciences ,020206 networking & telecommunications ,Astronomy and Astrophysics ,Field of view ,02 engineering and technology ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,Radio telescope ,Pathfinder ,Square kilometre array ,Space and Planetary Science ,0103 physical sciences ,0202 electrical engineering, electronic engineering, information engineering ,Systems design ,Aerospace engineering ,business ,Astrophysics - Instrumentation and Methods for Astrophysics ,010303 astronomy & astrophysics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) - Abstract
In this paper we describe the system design and capabilities of the Australian Square Kilometre Array Pathfinder (ASKAP) radio telescope at the conclusion of its construction project and commencement of science operations. ASKAP is one of the first radio telescopes to deploy phased array feed (PAF) technology on a large scale, giving it an instantaneous field of view that covers 31 square degrees at 800 MHz. As a two-dimensional array of 36x12m antennas, with baselines ranging from 22m to 6km, ASKAP also has excellent snapshot imaging capability and 10 arcsecond resolution. This, combined with 288 MHz of instantaneous bandwidth and a unique third axis of rotation on each antenna, gives ASKAP the capability to create high dynamic range images of large sky areas very quickly. It is an excellent telescope for surveys between 700 MHz and 1800 MHz and is expected to facilitate great advances in our understanding of galaxy formation, cosmology and radio transients while opening new parameter space for discovery of the unknown., 38 pages, 24 figures, accepted for publication in PASA
- Published
- 2021