; IDL Version 3.6.1a (sunos sparc)
; Journal File for gschneid@nicmosis
; Working directory: /home/gschneid/FILTERS/IDL-PROCS
; Date: Thu Aug 31 12:51:37 1995
 
;The Journal is /home/gschneid/FILTERS/SENSITIVITY/f190n-2CAM3.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: f190n-2
;The detector dark current in electrons per second is:      0.100000
;The linear range in electrons is:       205000.
;The wavelength interval in microns is:   0.000199601
;The effective filter bandwidth in microns is:    0.00441788
;Lower Wavelength is:       1.88220
;Upper Wavelength is:       1.92020
;Central Wavelength is:       1.90120
;Maximum Transmission is:      0.932236
;Lower half power wavelength is:       1.89160
;Upper half power wavelength is:       1.90920
;The average transmission between half power points is:      0.841107
;The background detected is      0.744488 photons per second
;The background from HST is      0.518144 photons per second
;The background from NICMOS is      0.168662 photons per second
;The background from zodiacal dust is     0.0576819 photons per second
; 
;The fraction of flux in the center pixel is:      0.564027
;