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The input flux wavelength distribution

In the expected count formula it is present the flux F term. This is determined by the input flux wavelength distribution. The user can select one out of several shapes. For example:

Blackbody
Template Spectra
Power Law
Continuum

Blackbody
Template Spectra
Power Law
Continuum
The effect of the object magnitude at a specific observation band
Single Line source

Pascal Ballester
1999-07-29