Author/Authors :
Pacciani، نويسنده , , Pier Luigi and Morelli، نويسنده , , Ennio and Rubini، نويسنده , , Alda and Mastropietro، نويسنده , , Marcello and Porrovecchio، نويسنده , , Geiland and Costa، نويسنده , , Enrico and Del Monte، نويسنده , , Ettore and Donnarumma، نويسنده , , Immacolata and Evangelista، نويسنده , , Yuri and Feroci، نويسنده , , Marco and Lazzarotto، نويسنده , , Francesco and Rapisarda، نويسنده , , Massimo and Soffitta، نويسنده , , Paolo، نويسنده ,
Abstract :
In this paper we describe the electronics of the SuperAGILE X-ray imager on-board AGILE satellite and the instrumentation developed to test and improve the Front-End and digital electronics of the flight model of the imager. Although the working principle of the instrument is very well established, and the conceptual scheme simple, the budget and mechanical constraints of the AGILE small mission made necessary the introduction of new elements in SuperAGILE, regarding both the mechanics and the electronics. In fact the instrument is contained in a ∼ 44 × 44 × 16 cm 3 volume, but the required performance is quite ambitious, leading us to equip a sensitive area of ∼ 1350 cm 2 with 6144 Silicon μ strips detectors with a pitch of 121 μ m and a total length of ∼ 18.2 cm . The result is a very light and power-cheap imager with a good sensitivity ( ∼ 15 m Crab in 1 day in 15 – 45 keV ), high angular resolution ( 6 arcmin ) and gross spectral resolution. The test-equipment is versatile, and can be easily modified to test FEE based on self-triggered, data-driven and sparse-readout ASICs such as XA family chips.
Keywords :
Silicon microstrip , Coded mask , Test instrumentation , X-ray imager , Gamma ray bursts