2016
DOI: 10.4018/978-1-5225-0242-5
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Position-Sensitive Gaseous Photomultipliers

Abstract: Advances in the technologies associated with position sensitive gaseous detectors especially featuring CsI as reflective photoconverters will be reviewed. These photodetectors represent the most effective solution for what concerns cost and performance in the case of large area Cherenkov imaging applications in relatively low rate (or low occupancy) high energy physics and astrophysics experiments. Moreover, they are the only choice when the Cherenkov detector is embedded in a magnetic field. Recently proposed… Show more

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Cited by 3 publications
(6 citation statements)
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“…As can be seen, depending on the specific design, the developed detectors have 10 2 ÷10 3 times larger sensitivity than the best commercial sensors. [6,[8][9][10] and confirmed by us [11]. Here we present the most important parameters, in particular relative sensitivity, whose method of measurement is explained in section 2.…”
Section: Jinst 15 T12001supporting
confidence: 61%
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“…As can be seen, depending on the specific design, the developed detectors have 10 2 ÷10 3 times larger sensitivity than the best commercial sensors. [6,[8][9][10] and confirmed by us [11]. Here we present the most important parameters, in particular relative sensitivity, whose method of measurement is explained in section 2.…”
Section: Jinst 15 T12001supporting
confidence: 61%
“…Measurements with a calibration cell show that the photo-current reaches a plateau at T > 80 • C. The QE of EF in full absorption (the region of the saturated photocurrent) is 𝑄 sat ≈ 20% at 190 nm [6]. Vapor pressure of EF at 80 • C and 40 • C, are about 2 and 0.2 Torr, respectively.…”
Section: Jinst 15 T12001mentioning
confidence: 95%
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