Photoreceiver efficiency measurements

Details Photoreceiver efficiency measurements Photoreceiver efficiency measurements

Jan 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7515975l&link_type=abstract

Unknown

Astronomy and Astrophysics

Astrophysics

Astrophysics, Lasers, Transmission Efficiency, Apertures, Astronomical Observatories, Block Diagrams, Oscilloscopes, Stellar Luminosity, Stellar Spectra

Scientific paper

The efficiency and other related parameters of Smithsonian Astrophysical Observatory's four laser receivers were measured at the observing stations by oscilloscope photography. If the efficiency is defined as the number of photoelectrons generated by the photomultiplier tube divided by the number of photons entering the aperture of the receiver, its measured value is about 1% for the laser wavelength of 694 nm. This value is consistent with the efficiency computed from the specified characteristics of the photoreceiver's optical components.

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