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Array noise performance


The following links are to maps of both SCUBA arrays with colour-coded circles representing noisy pixels. They are derived from an average over several weeks prior to the date listed, and should only be used as a guide to original (i.e. circa 1998) noise performance. Observers are still encouraged to take several NOISE REFERENCE observations per shift to determine current performance.

LW array noise map
SW array noise map

Contact: Remo Tilanus. Updated: Mon Mar 7 16:09:36 HST 2005

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