B. Butler, A. Wootten
October 25, 1999
Keywords: grating, infrared filter, analysis
This memo presents a calculation of the sensitivity of the ALMA array, given new thinking on number of antennas, resolutions of different configurations, and other considerations. Much of it is drawn from a similar calculation in Butler et al. (1999), which was patterned after Brown (1998). Numbers for the Supra-THz windows and baselines longer than 10 km are also presented and discussed.
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