1947
DOI: 10.1364/josa.37.000420
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Multiplier Photo-Tube Characteristics: Application to Low Light Levels*

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Cited by 206 publications
(23 citation statements)
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“…Also the area of saturation in the upper right corner retreated to some extent, which is likely to be caused by shorter decays limiting the space charge build-up time at the end of the dynode chain. [16][17][18] The lifetime gradient for low light intensities (present in Figure 8) has vanished and some elements at low gains and intensities remained empty due to signal-to-noise (S/N) issues at shorter decays.…”
Section: Resultsmentioning
confidence: 99%
“…Also the area of saturation in the upper right corner retreated to some extent, which is likely to be caused by shorter decays limiting the space charge build-up time at the end of the dynode chain. [16][17][18] The lifetime gradient for low light intensities (present in Figure 8) has vanished and some elements at low gains and intensities remained empty due to signal-to-noise (S/N) issues at shorter decays.…”
Section: Resultsmentioning
confidence: 99%
“…With a photodiode detector, the electrical noise is usually a parameter of the diode or its associated amplifier and is not greatly dependent upon the level of illumination. For a photomultiplier, however, the noise is mainly due to the photoelectric emission process and is proportional to the square root of the illumination [16,17].…”
Section: Photoelectric Detectionmentioning
confidence: 99%
“…If we assume that our receiver has a 1 .& filter before the detector, we find [from (8)] that it receives 2.4X1O-l1 W of noise from the background.…”
Section: System Bandwidth and Noisementioning
confidence: 99%