Jessica T. Dempsey, Wayne S. Holland, Antonio Chrysostomou, David S. Berry, Daniel Bintley, Edward L. Chapin, Simon C. Craig, Iain M. Coulson, Gary R. Davis, Per Friberg, Tim Jenness, Andy G. Gibb, Harriet A. L. Parsons, Douglas Scott, Holly S. Thomas, Remo P. J. Tilanus, Ian Robson, Craig A. Walther
SCUBA-2 is the largest submillimetre wide-field bolometric camera ever built. This 43 square arc-minute field-of-view instrument operates at two wavelengths (850 and 450 microns) and has been installed on the James Clerk Maxwell Telescope on Mauna Kea, Hawaii. SCUBA-2 has been successfully commissioned and operational for general science since October 2011. This paper presents an overview of the on-sky performance of the instrument during and since commissioning in mid-2011. The on-sky noise characteristics and NEPs of the 450 and 850 micron arrays, with average yields of approximately 3400 bolometers at each wavelength, will be shown. The observing modes of the instrument and the on-sky calibration techniques are described. The culmination of these efforts has resulted in a scientifically powerful mapping camera with sensitivities that allow a square degree of sky to be mapped to 10 mJy/beam rms at 850 micron in 2 hours and 60 mJy/beam rms at 450 micron in 5 hours in the best weather.
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http://arxiv.org/abs/1208.4622
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