Input Flux Distribution

 Uniform (constant with wavelength)
 Blackbody: T =		 Kelvin
 Template Spectra:	
O5V   (Kurucz)
 O5V (Pickles)
 O9V (Pickles)
B1V   (Kurucz)
B2IV  (Pickles)
B3V   (Kurucz)
B8V   (Kurucz)
B9III (Pickles)
B9V (Pickles)
A0III (Pickles)
 A0V (Pickles)
A1V   (Kurucz)
F0V   (Kurucz)
G0    (Pickles)
G2V   (Kurucz)
K2V   (Pickles)
K7V   (Pickles)
M2V   (Pickles)
Planetary Nebula
HII Region (ORION)
Elliptical Galaxy
S0 Galaxy
Sa Galaxy
Sb Galaxy
Starburst Galaxy 1
Starburst Galaxy 2
Starburst Galaxy 3
Starburst Galaxy 4
Starburst Galaxy 5
Starburst Galaxy 6
E Galaxy (GALEV)
QSO
  Redshift Z = 

  Object Magnitude:       		Band: 
U
B
V
R
I


Magnitudes are given per square arcsec for extended sources. Note that some template spectra are 
defined over a limited wavelength range and may not allow calculations for all instrument configurations. 

The object magnitude is not taken into account for the following single line source
 Single line
	Wavelength:         nm
	Flux:               10-16 ergs/s/cm2 (per arcsec2 for extended sources)
	FWHM:               nm (Minimum value: 0.50)

Spatial Distribution:	 Point Source		 Extended Source
Sky Conditions
Days From New Moon: 
0 days3 days
7 days10 days
14 days
 Airmass:    Seeing:  arcsec
The sky brightness is determined by the moon phase and the instrument efficiency according to this table.

Instrumental Setup

  

    
Filter:
    
    

          
			 640 U Bessel
			 639 B Bessel
			641 V Bessel
			 642 R Bessel
			 782 gunn g
			 786 gunn r
			 705 gunn i
			 623 gunn z
			 692 H alpha
			 709 H alpha Red
			 742 H beta Red
			 743 Hbe Cont
			 687 [OIII]
			 700 [SII]
			 724 Tyson B
          
    
  
  

    
Detector:  CCD#40
 
    
Readout mode:
                                 slow
                                 normal
                                 fast
                     
                    Binning:
                                 1x1
                                 2x2
                                 3x3
                                 4x4                                 
                                
    
  
   
  

    
 Polarimetry Mode: 	
    
    

    No polarimetry Linear or circular polarisation 
    
  



Results
 S/N:			Value    Plotting range  %
 Exposure Time (s):	Value    Plotting range  %

On submission the model can generate the following graphs:
 Input spectrum in physical units
 Total Efficiency
 CCD Illumination
 S/N as a function of Seeing
 S/N as a function of Exposure Time




           











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