The Variable Radio Sky from the Allen Telescope Array

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Scientific paper

The Allen Telescope Array (ATA) is, among other projects, undertaking large surveys of the radio sky at 1.4 and 3.14 GHz. With its wide field of view (about 5 square degrees at 1.4 GHz), the ATA is one of the most powerful radio survey telescopes in the world. As well as quantifying variability of radio sources using many epochs of imaging, and exploring new areas of area -- depth -- cadence parameter space in the search for radio transients, we are undertaking multi-wavelength studies (e.g. simultaneous optical observations of nearby galaxy nuclei using the Kepler satellite) to better probe the physical processes driving variability.

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