The next generation of radio arrays are being designed under the umbrella of the “Square Kilometer Array” (SKA) project. The leading concept for a “mid‐frequency” (0.3–10 GHz) array is a large wide‐field Radio Synoptic SKA (RSSKA), which is being developed for presentation to the upcoming Astronomy and Astrophysics Decadal Survey. The RSSKA is targeted at obtaining HI observations of a billion galaxies to redshift over 10000 square degrees, and synoptic mapping of the radio sky for transient detection and monitoring. In this talk I discuss the motivation for and the design challenges facing the RSSKA. Also suggested is a path forward from our current generation of facilities, such as the VLA and Arecibo, towards construction and operation of the RSSKA.
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1 August 2008
THE EVOLUTION OF GALAXIES THROUGH THE NEUTRAL HYDROGEN WINDOW
1–3 February 2008
Arecibo Observatory (Puerto Rico)
Research Article|
August 01 2008
The road to the Radio Synoptic SKA (RSSKA)
Steven T. Myers
Steven T. Myers
National Radio Astronomy Observatory, P.O. Box O, Socorro, NM, 87801
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Steven T. Myers
National Radio Astronomy Observatory, P.O. Box O, Socorro, NM, 87801
AIP Conf. Proc. 1035, 310–317 (2008)
Citation
Steven T. Myers; The road to the Radio Synoptic SKA (RSSKA). AIP Conf. Proc. 1 August 2008; 1035 (1): 310–317. https://doi.org/10.1063/1.2973607
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