|
HOME
ESR
EXPERIMENTS
LABS etc
|
|
E121
E127
E132
E125
E143
laser_cooling_2021
E142
Ê128
E146
E0052
E0018
E0028
E0038
E0075
E0203_E0018
E0052_2025
|
| Nuclear hyperfine mixing in 229Th89+ 2025 |
Not logged in |
 |
|
|
|
|
Message ID: 4
Entry time: Wed Jun 4 16:18:57 2025
In reply to: 1
|
| Author: |
Rodolfo, Simon |
| Category: |
Detectors |
| Subject: |
PMT dark count rates |
|
|
I adjusted the offsets of the amplifiers in the cave and measured the dark count rates :
|
PMT | Model | | Operation Voltage | Count rate (Hz)
| |
South | ET9422B | Broadband | -1500 V | 1300
| |
Middle | ET9423B | Smallband | -2650 V | 20
| |
North | ET9423B | Smallband | -2650 V | 30
|
Also the MCP anode of the XUV detector is now connected to the amplifiers and fed to the data cable of "PMT Cu".
| Quote: | This is the arrangement of the photomultipiers at the optical detection region at ESR for Thorium 2025
|
PMT | Model | SN | | Operation Voltage | Threshold
| |
South | ET9422B | 1042 | Broadband | -1500 V |
| |
Middle | ET9423B | 653 | Smallband | -2650 V | 10 (preliminary)
| |
North | ET9423B | 652 | Smallband | -2650 V | 12 (preliminary)
| |
|
|
|