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The Square Kilometre Array

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arxiv 1105.5953 v1 pith:7MQMUOI6 submitted 2011-05-30 astro-ph.IM

Steve Rawlings , Richard Schilizzi This is my paper · ORCID
classification astro-ph.IM
keywords arraykilometresquareamongstareasastronomicalastronomybeyond
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We review the current status of the Square Kilometre Array (SKA) by outlining the science drivers for its Phase-1 (SKA1) and setting out the timeline for the key decisions and milestones on the way to the planned start of its construction in 2016. We explain how Phase-2 SKA (SKA2) will transform the research scope of the SKA infrastructure, placing it amongst the great astronomical observatories and survey instruments of the future, and opening up new areas of discovery, many beyond the confines of conventional astronomy.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Redshift drift effect through the observation of HI 21cm signal with SKA

    astro-ph.CO 2025-01 reject novelty 3.0 of 10

    A forecast study claims SKA with 0.001 Hz spectral resolution could measure cosmic redshift drift at millimeter-per-second precision over 0.5 years, yielding tight dark energy constraints.

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