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Detector Solid Angles

 Each detector is assumed to have the following effective solid angle (in units of 1.0E-7 steradians):

    #1     #2     #3     #4     #5     #6     #7     #8     #9
   14.1,  13.7,  12.9,  13.1,  13.2,  13.2,  13.6,  6.10,  6.04,  

    #10    #11    #12    #13    #14    #15    #16    #17    #18
   6.07,  1.92,  4.85,  6.10,  6.19,  6.56,  3.39,  DEAD   3.46,  

    #19    #20    #21    #22    #23    #24    #25    #26    #27
   3.40,   DEAD  3.48,  3.38,  3.21,  3.22,  3.17,  0.92,  2.41,  

    #28    #29    #30    #31    #32    #33    #34    #35    #36
   2.95,  3.25,  3.25,  1.97,  6.40,  6.32,  6.25,  6.36,   DEAD  

    #37    #38    #39    #40    #41    #42    #43    #44    #45
   6.37,  4.84,  1.82,  3.50,  3.44,  3.48,  3.50,  3.45,  3.46,  

    #46    #47    #48    #49    #50    #51    #52    #53    #54
   1.78,  0.89,  3.31,  3.22,  3.29,  3.25,  3.19,  3.24,  2.45,

    #55    #56    #57    #58    #59    #60    #61    #62
    7.9,  13.3,  14.0,  12.9,  14.0,  13.8,  14.2,   6.8

These values were derived by M. Moshir at the Infrared Processing and Analysis Centre (IPAC), CalTech, and are consistent with the detector Point Spread Functions used by IRAS90 (see section [*]).



next up previous contents
Next: Point Spread Functions
Up: Using IRAS90 - Details
Previous: Detector Bandwidths

IRAS90 --- IRAS Survey and PO Data Analysis Package --- Reference Guide
Starlink User Note 163
David S. Berry, W Gong, D C Parsons
19 February 1995
E-mail:ussc@star.rl.ac.uk

Copyright © 2008 Science and Technology Facilities Council