The next generation of high-energy gamma-ray detectors for satellites: The AGILE silicon tracker
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5 pages
Part of Gamma-ray astrophysics. Proceedings, Symposium, Gamma 2001, Baltimore, USA, April 4-6, 2001, 754
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- AIP Conf.Proc. 587 (2001) 1, 754
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- Published: Feb 20, 2002
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Abstract: (AIP)
AGILE (Light Imaging Detector for Gamma Astronomy) is a satellite for the detection of gamma-ray sources in the energy range 30 MeV–50 GeV within a large field of view (∼1/5 of the sky) and it is planned to fly in the years 2003–2006, a period in which no other mission entirely dedicated to photon detection above 30 MeV is planned. AGILE is made of a Tungsten-Silicon Tracker, a CsI Minicalorimeter, an anticoincidence system and a X-ray detector sensitive in the 10–40 keV range. The Tracker consists of 14 planes, each one made of 2 layers of 16 single-sided, AC coupled, 410 μm thick, 9.5×9.5 cm2 Silicon detectors with a readout pitch of 242 μm and a floating strip. The AGILE trigger is generated by the Silicon strips which are readout by the TAAI, a low noise, self triggering ASIC used in a very low power configuration (∼400 μW/channel) with analog readout. The number of Tracker readout channels is 43000. We present a description of the Tracker and the performance of the detector (position resolution, cluster pulse height, readout and trigger logic) obtained during three testbeam periods at CERN.- talk: Baltimore 2001/04/04
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