Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992spie.1743..192s&link_type=abstract
In: EUV, X-ray, and gamma-ray instrumentation for astronomy III; Proceedings of the Meeting, San Diego, CA, July 22-24, 1992 (A9
Astronomy and Astrophysics
Astronomy
Charge Coupled Devices, Satellite-Borne Instruments, Windows (Apertures), X Ray Detectors, X Ray Imagery, X Ray Spectroscopy, Environmental Tests, Filters, Optical Properties, Thermal Stresses, Transmittance, Vibration Tests
Scientific paper
A prototype spectral filter was developed to be used as a radiation entrance window for a satellite borne CCD X-ray imaging detector, which is presently under development within the EOBB (Electro-Optical-Breadboard) phase of ESA's X-ray Multimirror Mission project. CCDs have a broad spectral response ranging from the X-ray to the NIR range. For X-ray observations, the filter being located in front of the detector must suppress the radiation of visible and UV stars by more than 6 orders of magnitude, and be highly transparent at energies above 0.1 keV. The technique to manufacture the windows and the measurements of the spectral transmittance as well as the environmental testing is described. Performance data are given.
Braeuninger Heinrich
Frischke Dagmar
Krumrey Michael
Maier Hans-Joerg
Mueller Peter
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