8-dec-1997
Case 0: Compact Source, 2 footpoints, 20 arcsec separation. Ideal conditions, E = 500 keV, 10 counts/sec-keV totaled for all detectors DT = 300 sec, DE = 60 keV. Zero background,
Case 1: Compact Source, 2 footpoints, 20 arcsec separation. E = 500 keV, 10 counts/sec-keV totaled for all detectors, DT = 300 sec, DE = 60 keV. Signal to noise ratio is 14. Images have 2 arcsec pixels.
Case 2: Compact Source, 2 footpoints, 20 arcsec separation. E = 500 keV, 4 counts/sec-keV totaled for all detectors, DT = 300 sec, DE = 80 keV. Signal to noise ratio is 5.7. Images have 2 arcsec pixels.
Case 3: Line Emission, Compact Source, 2 footpoints, 20 arcsec separation. E = 511 keV, 23 counts/sec-keV totaled for all detectors, DT = 300 sec, DE = 5 keV. Signal to noise ratio is 33. Images have 2 arcsec pixels.
Case 4: Line Emission, Compact Source, 2 footpoints, 20 arcsec separation. E = 511 keV, 9.2 counts/sec-keV totaled for all detectors, DT = 300 sec, DE = 5 keV. Signal to noise ratio is 13.1. Images have 2 arcsec pixels.
Case 5: Extended Source, 2 footpoints, with looptop source of 1/2 the total brightness. E = 500 keV, 10 counts/sec-keV totaled for all detectors, DT = 300 sec, DE = 60 keV. Zero background. Images have 4 arcsec pixels.
Case 6: Extended Source, 2 footpoints, with looptop source of 1/2 the total brightness. E = 500 keV, 10 counts/sec-keV totaled for all detectors, DT = 300 sec, DE = 60 keV. Signal to noise ratio is 14.3. Images have 4 arcsec pixels.
Case 7: Extended Source, 2 footpoints, with looptop source of 1/2 the total brightness. E = 500 keV, 4 counts/sec-keV totaled for all detectors, DT = 300 sec, DE = 80 keV. Signal to noise ratio is 5.7. Images have 4 arcsec pixels.
Case 8: Line Emission, Extended Source, 2 footpoints, with looptop source of 1/2 the total brightness. E = 511 keV, 23 counts/sec-keV totaled for all detectors, DT = 300 sec, DE = 5 keV. Signal to noise ratio is 33. Images have 4 arcsec pixels.
Case 9: Line Emission, Extended Source, 2 footpoints, with looptop source of 1/2 the total brightness. E = 511 keV, 9.2 counts/sec totaled for all detectors, DT = 300 sec, DE = 5 keV. Signal to noise ratio is 13.1. Images have 4 arcsec pixels.
Case 10: Line Emission, Compact Source, 2 footpoints, 20 arcsec separation. E = 2223 keV, 24.0 counts/sec-keV totaled for all detectors, DT = 300 sec, DE = 2.5 keV. Signal to noise ratio is 400. Images have 2 arcsec pixels.
Case 11: Line Emission, Compact Source, 2 footpoints, 20 arcsec separation. E = 2223 keV, 2.4 counts/sec-keV totaled for all detectors, DT = 300 sec, DE = 2.5 keV. Signal to noise ratio is 40. Images have 2 arcsec pixels.
Case 12: Line Emission, Extended Source, 2 footpoints, with
looptop source of 1/2 the total brightness. E = 2223 keV, 24.0
counts/sec-keV totaled for all detectors, DT = 300 sec, DE = 2.5 keV.
Signal to noise ratio is 400. Images have 4 arcsec pixels.
Case 13: Line Emission, Extended Source, 2 footpoints, with
looptop source of 1/2 the total brightness. E = 2223 keV, 2.40
counts/sec-keV totaled for all detectors, DT = 300 sec, DE = 2.5 keV.
Signal to noise ratio is 40. Images have 4 arcsec pixels.
Comments to: jimm@ssl.berkeley.edu
Written, 25-Nov-1997, jmm
