English

Novel Photo Multiplier Tubes for the Cherenkov Telescope Array Project

Instrumentation and Methods for Astrophysics 2019-08-14 v1 Instrumentation and Detectors

Abstract

Currently the standard light sensors for imaging atmospheric Cherenkov telescopes are the classical photo multiplier tubes that are using bialkali photo cathodes. About eight years ago we initiated an improvement program with the Photo Multiplier Tube (PMT) manufacturers Hamamatsu (Japan), Electron Tubes Enterprises (England) and Photonis (France) for the needs of imaging atmospheric Cherenkov telescopes. As a result, after about 40 years of stagnation of the peak Quantum Efficiency (QE) on the level of 25-27%, new PMTs appeared with a peak QE of 35%. These have got the name super-bialkali. The second significant upgrade has happened very recently, as a result of a dedicated improvement program for the candidate PMT for Cherenkov Telescope Array. The latter is going to be the next generation major instrument in the field of very high energy gamma astrophysics and will consist of over 100 telescopes of three different sizes of 23m, 12m and 4-7m, located both in southern and northern hemispheres. Now PMTs with average peak QE of approximately 40% became available. Also, the photo electron collection efficiency of the previous generation PMTs of 80- 90% has been enhanced towards 95-98% for the new ones. The after-pulsing of novel PMTs has been reduced towards the level of 0.02% for the set threshold of 4 photo electrons. We will report on the PMT development work by the companies Electron Tubes Enterprises and Hamamatsu Photonics K.K. show the achieved results and the current status.

Keywords

Cite

@article{arxiv.1307.5463,
  title  = {Novel Photo Multiplier Tubes for the Cherenkov Telescope Array Project},
  author = {Takeshi Toyama and Razmik Mirzoyan and Hugh Dickinson and Christian Fruck and Jürgen Hose and Hanna Kellermann and Max Knötig and Eckart Lorenz and Uta Menzel and Daisuke Nakajima and Reiko Orito and David Paneque and Thomas Schweizer and Masahiro Teshima and Tokonatsu Yamamoto},
  journal= {arXiv preprint arXiv:1307.5463},
  year   = {2019}
}

Comments

In Proceedings of the 33rd International Cosmic Ray Conference (ICRC2013), Rio de Janeiro (Brazil). All CTA contributions at arXiv:1307.2232

R2 v1 2026-06-22T00:54:51.689Z