Figure 3: left :Image of the SPI coded mask as seen by the IBIS/PICSIT detector , at 2.75 MeV. The radioactive source was at large incidence with respect to the IBIS telescope axis. right: Image of the structure holding the two JEM-X coded masks, as seen by IBIS/PICSIT also at 2.75 MeV. We can see on top of the image a part of the IBIS coded mask.
• Innovation for detection systems › Detectors for both infinite physics
• Department of Astrophysics (DAp) // UMR AIM • pas de titre
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