; IDL Version 3.6.1a (sunos sparc)
; Journal File for gschneid@nicmosis
; Working directory: /home/gschneid/FILTERS/IDL-PROCS
; Date: Wed Aug 30 16:55:11 1995
 
;The Journal is /home/gschneid/FILTERS/SENSITIVITY/f166n-3CAM3.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: f166n-3
;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:    0.00329099
;Lower Wavelength is:       1.64240
;Upper Wavelength is:       1.67580
;Central Wavelength is:       1.65910
;Maximum Transmission is:      0.872438
;Lower half power wavelength is:       1.64980
;Upper half power wavelength is:       1.66640
;The average transmission between half power points is:      0.766433
;The background detected is     0.0733414 photons per second
;The background from HST is     0.0153451 photons per second
;The background from NICMOS is    0.00390329 photons per second
;The background from zodiacal dust is     0.0540930 photons per second
; 
;The fraction of flux in the center pixel is:      0.616297
;