Author/Authors :
Barbiellini، نويسنده , , G and Fedel، نويسنده , , G and Liello، نويسنده , , F and Longo، نويسنده , , F and Pontoni، نويسنده , , C and Prest، نويسنده , , M and Tavani، نويسنده , , M and Vallazza، نويسنده , , E، نويسنده ,
Abstract :
AGILE (Light Imager for Gamma-ray Astrophysics) is a small scientific satellite for the detection of cosmic γ-ray sources in the energy range 30 MeV–50 GeV with a very large field of view (1/4 of the sky). It is planned to be operational in the years 2003–2006, a period in which no other γ-ray mission in the same energy range is foreseen.
art of the AGILE scientific instrument is a silicon–tungsten tracker made of 14 planes of single sided silicon detectors for a total of 43 000 readout channels. Each detector has a dimension of 9.5×9.5 cm2 and a thickness of 410 μm.
sent here a detailed description of the performance of the detector prototype during a testbeam period at the CERN PS in May 2000. The Tracker performance is described in terms of position resolution and signal-to-noise ratio for on and off-axis incident charged particles. The measured 40 μm resolution for a large range of incident angles will provide an excellent angular resolution for cosmic γ-ray imaging.
Keywords :
?-ray detector , Silicon detector , Satellite , Self triggering , Floating strip