An evaluation of gallium arsenide for detector applications in X-ray astronomy
Forthcoming, imaging X-ray telescopes cannot detect photons with energies above ~10KeV due to the limitations of current optics and silicon detectors. However, there are known to be X-ray emissions at higher energies from neutron stars, pulsars, black hole candidates, supernova remnants, active gala...
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University of Leicester
1997
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| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.696340 |