Title of article
Recent measurements on the Hamamatsu 13 in., R8055, PhotoMultiplier Tubes
Author/Authors
Tsagli، نويسنده , , S. and Aggouras، نويسنده , , G. and Anassontzis، نويسنده , , E.G. and Ball، نويسنده , , A.E. and Chinowsky، نويسنده , , W. and Fahrun، نويسنده , , E. and Grammatikakis، نويسنده , , G. and Green، نويسنده , , C. and Grieder، نويسنده , , P. and Katrivanos، نويسنده , , P. and Koske، نويسنده , , P. and Ludvig، نويسنده , , J. and Markopoulos، نويسنده , , E. and Minkowsky، نويسنده , , P. and Nygren، نويسنده , , D. and ، نويسنده ,
Pages
4
From page
511
To page
514
Abstract
The key component of NESTOR, the deep-sea Cherenkov neutrino telescope, built in the Mediterranean, NW of Greece, is the optical module. The NESTOR Optical Module employs a PhotoMultiplier Tube (PMT) in a transparent glass pressure housing. The Hamamatsu PMT R8055-01, 13 in. photomultiplier was selected for NESTOR to replace the old 15′′ Hamamatsu PMTs (R2018-03). Extensive tests have been made on the sensitivity, uniformity, time resolution and noise rates of 162 R8055-01 13 in. PMTs
Journal title
Astroparticle Physics
Record number
2029812
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