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Exposure Time Calculators
Formula Book
A.Modigliani, 29/07/99
Main formula
The input flux wavelength distribution
Blackbody
Template Spectra
Power Law
Continuum
The effect of the object magnitude at a specific observation band
Single Line source
Energy of each photon
The telescope surface
The exposure Time
The total efficiency
The slit trasmission factor
The factors
and
The sky contribution
The FWHM of the Image Quality profile
Example cases
SOFI-Spectroscopy
Point Source
Sky
FORS1-Spectroscopy
Point Source
Sky
ISAAC-Imaging
Point Source
Sky
SUSI2-Imaging
Point Source
Sky
UVES
Expected Object counts
Expected Sky counts
Signal To Noise Ratio
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Pascal Ballester
1999-07-29