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3.1 Basics
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A Detection Method for
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2. THE STATISTICAL RATE
3. MODELING A REALISTIC STELLAR OCCULTATION BY A KBO
Subsections
3.1 Basics
3.2 Discussion
3.2.1 What about an irregularly shaped object ?
3.2.2 Smoothing the occultation lightcurve on the star disk.
3.3 What could be finally detected thanks to diffraction ?
DESPA, Observatoire de Paris
2000-04-05
