Background simulations of the wide field imager of the ATHENA X-ray observatory

Background simulations of the wide field imager of the ATHENA X-ray observatory

The ATHENA X-ray Observatory-IXO is a planned multinational orbiting X-ray observatory with a focal length of 11.5 m. ATHENA aims to perform pointed observations in an energy range from 0.1 keV to 15 keV with high sensitivity. For high spatial and timing resolution imaging and spectroscopic observat...

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Bibliographische Detailangaben
Hauptverfasser: Hauf, S., Kuster, M., Pia, M. G., Hoffmann, D. H. H., Lang, P., Neff, S., Stefanescu, A., Struder, L.
Format: Tagungsbericht
Sprache:eng
Schlagworte:
Copper
Fluorescence
Nickel
Sensitivity
Silicon carbide
Tin
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Beschreibung
Zusammenfassung:The ATHENA X-ray Observatory-IXO is a planned multinational orbiting X-ray observatory with a focal length of 11.5 m. ATHENA aims to perform pointed observations in an energy range from 0.1 keV to 15 keV with high sensitivity. For high spatial and timing resolution imaging and spectroscopic observations the 640 × 640 pixels 2 large DePFET-technology based Wide field Imager (WFI) focal plane detector, providing a field of view of 18 arcsec will be the main detector. Based on the actual mechanics, thermal and shielding design we present estimates for the WFI cosmic ray induced background obtained by the use of Monte-Carlo simulations and possible background reduction measures.
ISSN:1082-3654
2577-0829
DOI:10.1109/NSSMIC.2011.6154609