; IDL Version 3.6.1a (sunos sparc)
; Journal File for gschneid@nicmosis
; Working directory: /home/gschneid/FILTERS/IDL-PROCS
; Date: Wed Aug 30 16:33:51 1995
 
;The Journal is /home/gschneid/FILTERS/SENSITIVITY/polshCAM1.txt
; 
;The temperature of the HST optics is:       293.000
;The temperature of the NICMOS optics is:       275.000
;The temperature of the zodiacal dust is:       265.000
;The emissivity of the HST is:      0.100000
;The emissivity of NICMOS is:      0.150000
;The effective HST telescope area in square meters is:       4.07000
;Efficiency including filter or grism but not detector is:      0.650000
;The detector noise in electrons is:       35.0000
;The required signal to noise is:       1.00000
; 
;STScI filter designation is: polsh
;The detector dark current in electrons per second is:      0.180000
;The linear range in electrons is:       184000.
;The wavelength interval in microns is:   0.000500357
;The effective filter bandwidth in microns is:     0.0346459
;Lower Wavelength is:      0.792500
;Upper Wavelength is:       1.30750
;Central Wavelength is:       1.05000
;Maximum Transmission is:      0.775990
;Lower half power wavelength is:      0.807000
;Upper half power wavelength is:       1.28250
;The average transmission between half power points is:      0.636618
;The background detected is     0.0585462 photons per second
;The background from HST is   3.00011e-07 photons per second
;The background from NICMOS is   4.09809e-08 photons per second
;The background from zodiacal dust is     0.0585459 photons per second
; 
;The fraction of flux in the center pixel is:      0.151215
;