Legacy version P95-phase2 (December 2014)
Provided for reference only!

Input Flux Distribution

 Uniform (constant with wavelength)
 Blackbody: Temperature:  Kelvin

Object Magnitude:  Vega  AB

 Single line
	Wavelength:  nm
	Flux:        10-16 ergs/s/cm2 (per arcsec2 for extended sources)
	FWHM:        nm 

Sky Conditions

Airmass 
Seeing   arcsec

Instrument Setup

Filter:

	 Wide Band:   
	J
	H
	Ks

	 Narrow Band: 
	1.06
	1.08
	1.19
	1.21
	1.26
	1.28
	1.64
	1.71
	2.07
	2.09
	2.13
	2.17
	2.19
	2.25
	2.29
	2.34


Objective:

	
		Large Field
		

Detector

DIT:  sec 

Results

 S/N ratio:             Plotting range:  %  

 Exposure Time settings:
                  NDIT:  Plotting range:  %
                  NINT: 

 Detector Illumination
 S/N as a function of Exposure Time
 Total Efficiency
 S/N as a function of seeing (only for point-source)
 Input spectrum in physical units