; IDL Version 3.6.1a (sunos sparc)
; Journal File for gschneid@nicmosis
; Working directory: /home/gschneid/FILTERS/IDL-PROCS
; Date: Wed Aug 30 16:56:25 1995
 
;The Journal is /home/gschneid/FILTERS/SENSITIVITY/f110w-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: f110w-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:   0.000500500
;The effective filter bandwidth in microns is:     0.0602932
;Lower Wavelength is:      0.780500
;Upper Wavelength is:       1.43050
;Central Wavelength is:       1.10550
;Maximum Transmission is:      0.949032
;Lower half power wavelength is:      0.803500
;Upper half power wavelength is:       1.39550
;The average transmission between half power points is:      0.810363
;The background detected is       2.01774 photons per second
;The background from HST is   0.000188116 photons per second
;The background from NICMOS is   3.14485e-05 photons per second
;The background from zodiacal dust is       2.01752 photons per second
; 
;The fraction of flux in the center pixel is:      0.668028
;