Figure 2: top left :Energy spectrum recorded by the SPI telescope of the fluorescence emission of molybdenum at 17 keV. bottom left : Image of the IBIS mask detected by ISGRI, at the same energy. top right: Energy spectrum recorded by the SPI telescope of the 2,75 MeV radiation resulting from the decay of the 24Na radioactive source. bottom right : Image of the IBIS mask detected by PICSIT also at 2.75 MeV.
• Innovation for detection systems › Detectors for both infinite physics
• Department of Astrophysics (DAp) // UMR AIM • pas de titre
PHoCEA DSM 2024 - Tous droits réservés - Mentions légales - Ce site utilise Twitter Bootstrap
Dernière mise à jour : Nov 19th, 2024
