1 / 7

properties of photomultiplier Hamatsu R7725 at room temperature

properties of photomultiplier Hamatsu R7725 at room temperature. Hans-Otto Meyer, 2/14/07. photomultipliers. I tested five Hamamatsu R7725 photomultipliers. measurements. LED pulser 467 nm f = 9835 Hz. PS777 amp. LRS 621 Discr, U D. LRS 4300 FERA ADC. Wiener USB crate contr.

elvis-morin
Download Presentation

properties of photomultiplier Hamatsu R7725 at room temperature

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. properties of photomultiplierHamatsu R7725at room temperature Hans-Otto Meyer, 2/14/07

  2. photomultipliers I tested five Hamamatsu R7725 photomultipliers

  3. measurements LED pulser 467 nm f = 9835 Hz PS777 amp LRS 621 Discr, UD LRS 4300 FERA ADC Wiener USB crate contr. LRS 2277 TDC UHV 7.05 mm dia. aperture R7725 30 cm stops common start UL trigger measured (for every light pulse delivered to photocathode: ● amplitude of anode output ● times (after light pulse) of up to 16 pulses within a T = 16.4 μs period (discriminator set below 1pe response) UHV set to make 1pe pulse height similar for different tubes Variable-amplitude LED pulser, every light pulse makes a trigger for each PM, took data with four different light levels, including no light at all

  4. ΔE amplitude spectrum #3378 UHV = 1800 V UL = 10.03 V λe = 2.03 2/9/07 example deduced: ● N0 total number of events (light flashes) ● λe avg. number of photoelectrons emitted from cathode (from a fit with sum of Gaussians, red line) ● ε relative quantum efficiency (λe for constant light intensity, arbitrarily normalized) ● ΔE/E (in %) energy resolution of tube

  5. example: #3378 UHV = 1800 V UL = 10.03 V λe = 2.03 2/9/07 after-pulses dark current initial event time distribution time after light flash (μs) deduced: ● ndarkrate of dark events (no light) ● q ≡ Ndark/N0/λe the probability to have an after-pulse after an event that makes an avg. of 1 photoelectron (verified that number of dark-pulses scales with avg. number of pe’s)

  6. time distributions vary ‘normal’ tubes (3378, 3379) (distributions are similar) time after light flash (μs) modified tubes (3692, 3693, 3694) (distributions are similar) initial pulse time after light flash (μs)

  7. summary Hamamatsu R7725

More Related