AIDA GELINA BRIKEN nToF CRIB ISOLDE CIRCE nTOFCapture DESPEC DTAS EDI_PSA 179Ta CARME StellarModelling DCF K40
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Entry  Sat May 18 01:41:45 2019, Nacher, Algora, gain check after the night 
Only PM3 showed an small jump. It seems that it has moved. Even after changing the HV cable. We will pay attention to it in the next days.

The others seem stable.

File after the night with 137Cs and 60C
Entry  Wed May 15 06:53:52 2019, Nacher Kiss Algora, HV setting 
EMPTY00      │0.0    V 1500.0 uA    0.5 V    0.5 uA Off               
│00.0000
DET01        │ 597.0 V 1500.0 uA  596.5 V   89.5 uA On                
Entry  Wed May 15 09:57:54 2019, Nacher, root file with 60Co and 137Cs 201905151432_137Cs60Co.root
For JL to play...
Entry  Sun Jun 9 03:59:40 2019, Many, some cable changes 
The cable of detector 8 was changed (long cable) to reduce the noise. The cable (long) of the reference detector was also changed.
Entry  Wed May 15 07:48:08 2019, Kiss Algora Nacher, Saturation and pulser Saturation_pulser.ods
Saturation and pulser position after calibration

EDy1 16801 25000
Entry  Mon Jun 10 13:02:16 2019, Jose, Pancho, Ale, background, Aida in 8x
Start: 21:03

Stop: 09:30
Entry  Mon Jun 10 09:58:42 2019, Jose, Ale, Gain matching Screenshot_from_2019-06-10_17-58-00.pngScreenshot_from_2019-06-10_17-57-56.png
We have corrected small gain changes by changing the HV of detectors. Attached are the new values
Entry  Mon Jun 10 10:01:17 2019, Jose, Ale, Co and Cs for new calibration 
Start: 17:57 ?

Stop:18:15
Entry  Sun Jun 9 04:03:38 2019, Jorge, Jose, Pancho, Alvaro, Kike, Ale, effect of the pulser in the low energy part of the anodes Screenshot_from_2019-06-09_14-27-37.pngScreenshot_from_2019-06-09_14-31-32.png
There is an effect if the pulser is at higher frequency in the low energy part of the anodes (apart from the funny situation that the scaler shows an
increase from 1.7 Khz to 8.5 kHz and the dynodes rate remain with the same rate)

The effect can be seen in the spectrum of the anodes. See screenshots in the attachment. First attachment (pulser at 10 Hz, second attachment
Entry  Fri Jun 7 08:47:17 2019, Jorge, Alvaro, Tom, Sunghan, Ale, Co source, test of AIDA/TAS syncronization 201906071728_60Co_AIDA_in.rootScreenshot_from_2019-06-07_17-09-21.pnggainMatchSi.png
Start: 16:50

Stop: 17:28

Root: 201906071728_60Co_AIDA_in.root
Entry  Fri Jun 7 12:35:14 2019, Jorge, Alvaro, Correlation time AIDA_DTAS for 60Co source AidaDTAS60CoTest.pdf
Files at mars /home/briken/190607AidaTasTest60Co
Entry  Sat Jun 8 04:22:39 2019, Jorge Alvaro, AIDA TAS correlation with 137Cs BetaTas137Cs.pngBetaGAmma137Cs.png
Files at mars /home/briken/190607AidaTasTest137Cs
For this experiment TAS Signal is stored 
Entry  Tue May 14 13:16:33 2019, JLT, Hardware setup 11x
 
Entry  Wed May 15 04:03:23 2019, JAR, Synchronization with AIDA working SyncProcedure.pdf
Synchronization with AIDA is working, see attached document to proceed.
Entry  Sun Jun 16 19:18:15 2019, Ela, Victor, root files from run 30 to run 45 6x
 
Entry  Sun Jun 16 21:43:36 2019, Ela, Victor, root file 1:30-3:30 190617_0325_100Sn_048.root
 
Entry  Sun Jun 16 21:44:38 2019, Ela, Victor, root file 3:30-5:30 190617_0528_100Sn_051.root
 
Entry  Sun Jun 16 23:37:18 2019, Ela, Victor, root file 3:30-5:30 190617_0528_100Sn_051.root
 
Entry  Sun Jun 16 23:37:47 2019, Ela, Victor, root file 5:30-7:30 190617_0730_100Sn_054.root
 
Entry  Sun Jun 16 07:08:10 2019, Ela, Sonja, Victor, Alejandro, problems in coincidence crystals-F11 Crystals_coincidence_F11.pngTAC_crystals_coincidence_F11.png
We have noticed that there is a problems in the coincidence Crystals-F11. The TAC shows a lot of counts. The
Crystals spectrum in coincidence with F11 do not. The time window of this coincidence is from-50 to 50 samples
and it should be from -180 to 300 samples to be centered in the peak of the TAC.
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