The Square Kilometre Array

Richard T. Schilizzi; Peter E. F. Dewdney; T. Joseph W. Lazio

doi:10.1117/12.786780

17 July 2008 The Square Kilometre Array

Richard T. Schilizzi, Peter E. F. Dewdney, T. Joseph W. Lazio

Proceedings Volume 7012, Ground-based and Airborne Telescopes II; 70121I (2008) https://doi.org/10.1117/12.786780
Event: SPIE Astronomical Telescopes + Instrumentation, 2008, Marseille, France

Abstract

The SKA will have a collecting area of up to one million square metres spread over at least 3000 km, providing a sensitivity 50 times higher than the Expanded Very Large Array, and an instantaneous field of view (FoV) of at least several tens of square degrees and possibly 250 square degrees. The SKA science impact will be widely felt in astroparticle physics and cosmology, fundamental physics, galactic and extragalactic astronomy, solar system science and astrobiology. In this paper, we describe the main features of the SKA, paying attention to the design activities around the world, and outline plans for the final design and phased implementation of the telescope.

Citation Download Citation

Richard T. Schilizzi, Peter E. F. Dewdney, and T. Joseph W. Lazio "The Square Kilometre Array", Proc. SPIE 7012, Ground-based and Airborne Telescopes II, 70121I (17 July 2008); https://doi.org/10.1117/12.786780

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