An introduction to blocked impurity band detectors

Details An introduction to blocked impurity band detectors An introduction to blocked impurity band detectors

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988itp..work..193g&link_type=abstract

In NASA, Ames Research Center, Second Workshop on Improvements to Photometry p 193 (SEE N89-13310 04-89)

Astronomy and Astrophysics

Astronomy

Detectors, Impurities, Photomultiplier Tubes, Spectral Bands, Accuracy, Astronomy, Light (Visible Radiation), Planets, Seismology, Stars

Scientific paper

Blocked impurity band detectors fabricated using standard silicon technologies offer the possibility of combining high sensitivity and high accuracy in a single detector operating in a low background environment. The solid state photomultiplier described by Petroff et al., which is a new type of blocked impurity band detector, offers even higher sensitivity as well as operation in the visible spectral region. The principle of operation and possible application of blocked impurity band detectors for stellar seismology and the search for extra-solar planets are described.

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