1978
DOI: 10.1016/0029-554x(78)90025-3
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Wavelength dependence of timing properties of the XP 2020 photomultiplier

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Cited by 8 publications
(5 citation statements)
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“…The probability that a photon is detected in the j th bin, p j , is proportional to the discrete convolution of the IRF and the model for the fluorescence decay given in eq . where j 0 is given by b = j 0 ϵ. The parameter b describes the linear shift between the instrument response function and the fluorescence decay. ,,, The probability that a photon is detected in the range t 1 ≤ t ≤ t max = t 1024 must be ∑ j p j = 1. We have, therefore …”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…The probability that a photon is detected in the j th bin, p j , is proportional to the discrete convolution of the IRF and the model for the fluorescence decay given in eq . where j 0 is given by b = j 0 ϵ. The parameter b describes the linear shift between the instrument response function and the fluorescence decay. ,,, The probability that a photon is detected in the range t 1 ≤ t ≤ t max = t 1024 must be ∑ j p j = 1. We have, therefore …”
Section: Discussionmentioning
confidence: 99%
“…The parameter b describes the linear shift between the instrument response function and the fluorescence decay. 1,3,32,33 The probability that a photon is detected in the range t 1 ≤ t ≤ t max = t 1024 must be ∑ j p j = 1. We have, therefore…”
Section: ■ Materials and Methodsmentioning
confidence: 99%
“…This shift parameter is necessary because the lower energy ("redder") fluorescence photons travel at a different speed through dispersive optics than the higher energy ("bluer") excitation photons that are used to generate the IRF in a scattering experiment. 1,38,39 The probability that a photon is detected in the range t 1 ≤ t ≤ t max = t 1024 must be ∑ j p j = 1. We therefore have…”
Section: ■ Materials and Methodsmentioning
confidence: 99%
“…The probability that a photon is detected in the j th bin, p j , is proportional to the convolution of the IRF and the model for the fluorescence decay. where j 0 is given by b = j 0 ϵ. b is a linear shift between the instrument response function and the fluorescence decay. This shift parameter is necessary because the lower energy (“redder”) fluorescence photons travel at a different speed through dispersive optics than the higher energy (“bluer”) excitation photons that are used to generate the IRF in a scattering experiment. ,, …”
Section: Methodsmentioning
confidence: 99%
“…This is because linear focused photomultipliers have a major advantage over side-on PMTs as there is a lower transit time dependence on the point of illumination of the photocathode. This has been measured as ∼ 13 ps mm −1 by Calligaris et al (1978) for an XP 2020 photomultiplier.…”
Section: Linear Focused Photomultipliersmentioning
confidence: 99%