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~ 10 km<br />
Détection de <strong>gamma</strong>s par les techniques Cerenkov atmosphériques<br />
Particle<br />
Shower<br />
n = 1.0003<br />
~ 100 m<br />
Focal Plane<br />
Intensity→ -ray energy<br />
Image Form / Stereo → Background rejection<br />
Image orientation → Angular origin<br />
13 . 11 . 08 Yvonne Becherini, APC Paris 10
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