Input Flux Distribution

 



 Continuum (Flat Spectra)
 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)
GALEV Elliptical Galaxy
GALEV Sa Galaxy
GALEV Sb Galaxy
GALEV Sc Galaxy
GALEV Sd Galaxy
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
QSO
  Redshift Z = 

   Single line
	Wavelength:         nm
	Flux:               10-16 ergs/s/cm2 (per arcsec2 for extended sources)
	FWHM:               nm (Minimum value: 0.50)

 Object Magnitude:       		Band: 
U
B
V
R
I

Filter:             
U
B
V
R
I
z


Detector: 
               
               
                Low Gain
                

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

  Flat Field Accuracy: 0.0  

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 (for pointlike sources only)
 S/N as a function of Exposure Time
 2D simulated image (pointlike sources only)