People | Locations | Statistics |
---|---|---|
Naji, M. |
| |
Motta, Antonella |
| |
Aletan, Dirar |
| |
Mohamed, Tarek |
| |
Ertürk, Emre |
| |
Taccardi, Nicola |
| |
Kononenko, Denys |
| |
Petrov, R. H. | Madrid |
|
Alshaaer, Mazen | Brussels |
|
Bih, L. |
| |
Casati, R. |
| |
Muller, Hermance |
| |
Kočí, Jan | Prague |
|
Šuljagić, Marija |
| |
Kalteremidou, Kalliopi-Artemi | Brussels |
|
Azam, Siraj |
| |
Ospanova, Alyiya |
| |
Blanpain, Bart |
| |
Ali, M. A. |
| |
Popa, V. |
| |
Rančić, M. |
| |
Ollier, Nadège |
| |
Azevedo, Nuno Monteiro |
| |
Landes, Michael |
| |
Rignanese, Gian-Marco |
|
Trifoglio, M.
in Cooperation with on an Cooperation-Score of 37%
Topics
Publications (6/6 displayed)
- 2014DAS: A Data Management System for Instrument Tests and Operations
- 2014CIWS-FW: A Customizable Instrument Workstation Software Framework for Instrument-independent Data Handling
- 2009SuperAGILE Data Processing Services
- 2006The Mini-Calorimeter detector for the AGILE missioncitations
- 2004The Test Equipment of the AGILE Minicalorimeter Prototype
- 2004AGILE, a satellite for high energy γ-ray astrophysics: prospects for the Mini-Calorimetercitations
Places of action
Organizations | Location | People |
---|
article
AGILE, a satellite for high energy γ-ray astrophysics: prospects for the Mini-Calorimeter
Abstract
Astrorivelatore Gamma ad Immagini LEggero (AGILE) is an Italian Space Agency (ASI) small space mission for high energy astrophysics in the γ-ray energy range 30 MeV-50 GeV and in the X-ray band 10-40 keV. AGILE is composed of three scientific detectors: a Tungsten-Silicon Tracker, a CsI Mini-Calorimeter and a silicon based X-ray detector (Super-Agile), moreover, an anticoincidence system carries out background rejection. The satellite's payload will have good imaging performances (with angular resolution of a few arc-minutes in the γ-ray band), good timing resolution and a large field of view (about 1/5 of the sky). AGILE detection principle is based on the pair production process, that arises from the interaction between high energy photons and the tungsten layers of the Silicon Tracker. The Silicon Tracker is designed to determine the direction of the incoming radiation, while the Mini-Calorimeter evaluates the energy of the interacting photons. The Mini-Calorimeter can also work as a stand-alone γ-ray detector in the energy range 250 keV-250 MeV, with no imaging capabilities, for the detection of transients and γ-ray burst events (in cooperation with Super-Agile) and for the evaluation of γ-ray background fluctuations. In this paper a description of the Mini-Calorimeter is done.