| ID |
Date |
Author |
Subject |
|
15
|
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
201905180939_137Cs60Co_calib.root |
|
5
|
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 │00.0001
DET02 │ 548.5 V 1500.0 uA 548.0 V 82.5 uA On │00.0002
DET03 │ 526.0 V 1500.0 uA 526.0 V 79.0 uA On │00.0003
DET04 │ 697.0 V 1500.0 uA 696.5 V 105.0 uA On │00.0004
DET05 │ 449.5 V 1500.0 uA 449.0 V 67.0 uA On │00.0005
DET06 │ 820.0 V 1500.0 uA 820.5 V 123.0 uA On │00.0006
DET07 │ 558.0 V 1500.0 uA 558.0 V 84.0 uA On │00.0007
DET08 │ 486.0 V 1500.0 uA 486.0 V 73.5 uA On │00.0008
EMPTY09 │ 0.0 V 1500.0 uA 1.0 V 0.5 uA Off │00.0009
EMPTY10 │ 0.0 V 1500.0 uA 0.5 V 0.0 uA Off │00.0010
EMPTY11 │ 0.0 V 1500.0 uA 1.0 V 0.5 uA Off │00.0011
EMPTY12 │ 0.0 V 1500.0 uA 0.0 V 0.0 uA Off │02.0000
DET11 │ 576.5 V 300.0 uA 576.5 V 86.0 uA On │02.0001
DET12 │ 505.0 V 300.0 uA 505.5 V 75.5 uA On │02.0002
DET13 │ 620.0 V 300.0 uA 620.0 V 92.0 uA On │02.0003
DET14 │ 650.0 V 300.0 uA 650.0 V 96.5 uA On │02.0004
DET15 │ 653.5 V 300.0 uA 653.5 V 97.0 uA On │02.0005
DET16 │ 530.0 V 300.0 uA 529.5 V 78.5 uA On │02.0006
DET17 │ 462.5 V 300.0 uA 462.0 V 68.0 uA On │02.0007
DET18 │ 518.0 V 300.0 uA 518.0 V 77.5 uA On │02.0008
EMPTY19 │ 0.0 V 300.0 uA 0.0 V 0.0 uA Off │02.0009
EMPTY20 │ 0.0 V 300.0 uA 0.0 V 0.0 uA Off │02.0010
REF01 │800.0 V 300.0 uA 800.0 V 174.0 uA On │02.0011
|
|
8
|
Wed May 15 09:57:54 2019 |
Nacher | root file with 60Co and 137Cs |
For JL to play... |
| Attachment 1: 201905151432_137Cs60Co.root
|
|
106
|
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. |
|
6
|
Wed May 15 07:48:08 2019 |
Kiss Algora Nacher | Saturation and pulser |
Saturation and pulser position after calibration
EDy1 16801 25000
EDy2 18412 not seen
EDy3 25520 not seen
EDy4 15563 not seen
EDy5 22920 not seen
EDy6 13965 not seen
EDy7 17440 28000?
EDy8 17300 28000?
EDy11 14220 22293
EDy12 21824 not seen
EDy13 16750 not seen
EDy14 22230 not seen
EDy15 17505 not seen
EDy16 24955 not seen
EDy17 14250 29590
EDy18 26144 not seen |
| Attachment 1: Saturation_pulser.ods
|
|
116
|
Mon Jun 10 13:02:16 2019 |
Jose, Pancho, Ale | background, Aida in |
Start: 21:03
Stop: 09:30
Comment: no sources around
Root: 20190611_0930_background_AIDA_in.root
Figures: alignment of first half(1), alignment of second half(2), then comparison of detectors 1,11; 2,12;3,13; 5,15; 7,17
Clearly the contamination of the side of AIDA is seen (detectors 5,3)
|
| Attachment 1: 20190611_0930_background_AIDA_in.root
|
|
111
|
Mon Jun 10 09:58:42 2019 |
Jose, Ale | Gain matching |
We have corrected small gain changes by changing the HV of detectors. Attached are the new values |
| Attachment 1: Screenshot_from_2019-06-10_17-58-00.png
|
|
| Attachment 2: Screenshot_from_2019-06-10_17-57-56.png
|
|
|
112
|
Mon Jun 10 10:01:17 2019 |
Jose, Ale | Co and Cs for new calibration |
Start: 17:57 ?
Stop:18:15
Comment: We put Co and Cs on top of each other below AIDA in the center of the DTAS with the help of the plastic
ruler.
Root: 20190610_1815_60Co_137Cs_AIDA_in.root
To calibrate use the
[dacq@IFICdaq DRikenPreparation]$ root -l
root [0] .L calibrateEFIR_new.cxx
root [3] calibrateEFIR("20190610_1815_60Co_137Cs_AIDA_in.root")
An01_EFIR 306750 536250 606750
An02_EFIR 281250 489750 554250
An03_EFIR 282750 491250 557250
An04_EFIR 263250 458250 518250
An05_EFIR 270750 471750 534750
An06_EFIR 308250 537750 609750
An07_EFIR 290250 506250 572250
An08_EFIR 284250 495750 560250
An11_EFIR 365250 636750 722250
An12_EFIR 263250 459750 521250
An13_EFIR 321750 560250 635250
An14_EFIR 327750 572250 648750
An15_EFIR 300750 522750 591750
An16_EFIR 287250 500250 567750
An17_EFIR 296250 516750 585750
An18_EFIR 273750 479250 542250
Dy01_EFIR 34296.9 59765.6 67578.1
Dy02_EFIR 33828.1 59140.6 66953.1
Dy03_EFIR 34140.6 59296.9 67109.4
Dy04_EFIR 34140.6 59453.1 67265.6
Dy05_EFIR 34453.1 59921.9 67890.6
Dy06_EFIR 34140.6 59453.1 67421.9
Dy07_EFIR 34453.1 60078.1 68046.9
Dy08_EFIR 33828.1 59140.6 66796.9
Dy11_EFIR 34453.1 60078.1 68203.1
Dy12_EFIR 34296.9 59765.6 67890.6
Dy13_EFIR 34296.9 59765.6 67578.1
Dy14_EFIR 34296.9 59921.9 67890.6
Dy15_EFIR 34140.6 59765.6 67578.1
Dy16_EFIR 34296.9 59765.6 67578.1
Dy17_EFIR 34296.9 59921.9 67734.4
Dy18_EFIR 33984.4 59453.1 67265.6
An01_EFIR 306750 536250 606750 0.00223435 -23.9647
An02_EFIR 281250 489750 554250 0.00245634 -29.3018
An03_EFIR 282750 491250 557250 0.00244617 -29.701
An04_EFIR 263250 458250 518250 0.0026289 -30.6075
An05_EFIR 270750 471750 534750 0.00254201 -26.4752
An06_EFIR 308250 537750 609750 0.00222596 -24.3613
An07_EFIR 290250 506250 572250 0.00237623 -28.3674
An08_EFIR 284250 495750 560250 0.00242761 -28.7476
An11_EFIR 365250 636750 722250 0.00188032 -24.9273
An12_EFIR 263250 459750 521250 0.00260091 -22.9409
An13_EFIR 321750 560250 635250 0.00214105 -27.0487
An14_EFIR 327750 572250 648750 0.00209042 -23.3901
An15_EFIR 300750 522750 591750 0.00230503 -31.6127
An16_EFIR 287250 500250 567750 0.002394 -25.7022
An17_EFIR 296250 516750 585750 0.00231789 -24.9283
An18_EFIR 273750 479250 542250 0.00249619 -21.9428
Dy01_EFIR 34296.9 59765.6 67578.1 0.020139 -29.3045
Dy02_EFIR 33828.1 59140.6 66953.1 0.0202412 -23.2189
Dy03_EFIR 34140.6 59296.9 67109.4 0.0203445 -32.9624
Dy04_EFIR 34140.6 59453.1 67265.6 0.0202412 -29.5443
Dy05_EFIR 34453.1 59921.9 67890.6 0.020068 -29.6613
Dy06_EFIR 34140.6 59453.1 67421.9 0.0201694 -26.741
Dy07_EFIR 34453.1 60078.1 68046.9 0.0199676 -26.3096
Dy08_EFIR 33828.1 59140.6 66796.9 0.020313 -25.9882
Dy11_EFIR 34453.1 60078.1 68203.1 0.0198974 -23.544
Dy12_EFIR 34296.9 59765.6 67890.6 0.0199969 -23.7359
Dy13_EFIR 34296.9 59765.6 67578.1 0.020139 -29.3045
Dy14_EFIR 34296.9 59921.9 67890.6 0.0199676 -23.1897
Dy15_EFIR 34140.6 59765.6 67578.1 0.0200376 -22.8024
Dy16_EFIR 34296.9 59765.6 67578.1 0.020139 -29.3045
Dy17_EFIR 34296.9 59921.9 67734.4 0.0200376 -25.9333
Dy18_EFIR 33984.4 59453.1 67265.6 0.020139 -23.0111 |
|
107
|
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 |
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 pulser at 100 Hz) |
| Attachment 1: Screenshot_from_2019-06-09_14-27-37.png
|
|
| Attachment 2: Screenshot_from_2019-06-09_14-31-32.png
|
|
|
101
|
Fri Jun 7 08:47:17 2019 |
Jorge, Alvaro, Tom, Sunghan, Ale | Co source, test of AIDA/TAS syncronization |
Start: 16:50
Stop: 17:28
Root: 201906071728_60Co_AIDA_in.root
Comment: 60Co source on top of AIDA (red box, key 3). It is positioned on a plastic ruler in the center of the DTAS.
File Number Aida: R18 (_0 should not be used, reset of the time stamp was done during this file). R18_1 started at 16:57, last file R18_4
File Number DTAS: 245,247
201906071650_60Co_AIDA_245.dlt,... 201906071650_60Co_AIDA_247.dlt
After checking the shifts in gain, it seems that for most of the detectors the dynode and anode signal moved in the same direction with the exception of detector 13 (dynode and anode do not move
equally, so probably there is a cable problem here, probably in the Dynode 13 or preamp problem)
Edit 13/06/19 Oscar Hall
The low energy channels of AIDA have been gain matched. Attached is the energy plot of the x and y side strops in AIDA. |
| Attachment 1: 201906071728_60Co_AIDA_in.root
|
| Attachment 2: Screenshot_from_2019-06-07_17-09-21.png
|
|
| Attachment 3: gainMatchSi.png
|
|
|
103
|
Fri Jun 7 12:35:14 2019 |
Jorge, Alvaro | Correlation time AIDA_DTAS for 60Co source |
Files at mars /home/briken/190607AidaTasTest60Co |
| Attachment 1: AidaDTAS60CoTest.pdf
|
|
|
104
|
Sat Jun 8 04:22:39 2019 |
Jorge Alvaro | AIDA TAS correlation with 137Cs |
Files at mars /home/briken/190607AidaTasTest137Cs
For this experiment TAS Signal is stored |
| Attachment 1: BetaTas137Cs.png
|
|
| Attachment 2: BetaGAmma137Cs.png
|
|
|
2
|
Tue May 14 13:16:33 2019 |
JLT | Hardware setup |
|
| Attachment 1: DTAS-setup.png
|
|
| Attachment 2: DTAS-shielding.pdf
|
|
| Attachment 3: InnerSuportFrame.pdf
|
|
| Attachment 4: DTAS-assembly.png
|
|
| Attachment 5: DTAS-module.png
|
|
| Attachment 6: DTAS-PMT.pdf
|
|
| Attachment 7: DTAS-VD.pdf
|
|
| Attachment 8: WellDetector.png
|
|
| Attachment 9: WellDetector-PMT.pdf
|
|
| Attachment 10: MSI-8-P.pdf
|
|
| Attachment 11: 6010_datasheet.pdf
|
|
|
3
|
Wed May 15 04:03:23 2019 |
JAR | Synchronization with AIDA working |
Synchronization with AIDA is working, see attached document to proceed. |
| Attachment 1: SyncProcedure.pdf
|
|
|
133
|
Sun Jun 16 19:18:15 2019 |
Ela, Victor | root files from run 30 to run 45 |
|
| Attachment 1: 190617_0124_100Sn_045.root
|
| Attachment 2: 190616_2316_100Sn_042.root
|
| Attachment 3: 190616_2241_100Sn_041.root
|
| Attachment 4: 190616_2041_100Sn_038.root
|
| Attachment 5: 190616_1840_100Sn_035.root
|
| Attachment 6: 190616_1641_100Sn_032.root
|
|
134
|
Sun Jun 16 21:43:36 2019 |
Ela, Victor | root file 1:30-3:30 |
|
| Attachment 1: 190617_0325_100Sn_048.root
|
|
135
|
Sun Jun 16 21:44:38 2019 |
Ela, Victor | root file 3:30-5:30 |
|
| Attachment 1: 190617_0528_100Sn_051.root
|
|
138
|
Sun Jun 16 23:37:18 2019 |
Ela, Victor | root file 3:30-5:30 |
|
| Attachment 1: 190617_0528_100Sn_051.root
|
|
139
|
Sun Jun 16 23:37:47 2019 |
Ela, Victor | root file 5:30-7:30 |
|
| Attachment 1: 190617_0730_100Sn_054.root
|
|
131
|
Sun Jun 16 07:08:10 2019 |
Ela, Sonja, Victor, Alejandro | problems in coincidence crystals-F11 |
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.
We will change it at soon as possible |
| Attachment 1: Crystals_coincidence_F11.png
|
|
| Attachment 2: TAC_crystals_coincidence_F11.png
|
|