AIDA GELINA BRIKEN nToF CRIB ISOLDE CIRCE nTOFCapture DESPEC DTAS EDI_PSA 179Ta CARME StellarModelling DCF K40
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  ID Date Author Subjectdown
  117   Tue Jun 11 01:45:55 2019 Pancho, Alebackground
Start: 09:46

Stop: 13:49

Background, Aida in, no sources around, no beam

Root file: 20190611_1349_background_AIDA_in.root
Attachment 1: 20190611_1349_background_AIDA_in.root
  1   Tue May 14 09:41:24 2019 TDWelcome to the DTAS Elog
  127   Sun Jun 16 02:07:29 2019 VictorTotal sum (black) and anodes

Different cuts at high energy in individual spectra (anodes) and effect in the total sum

Attachment 1: SUM_and_individuals_anodes_cut8MeV.png
SUM_and_individuals_anodes_cut8MeV.png
Attachment 2: SUM_and_individuals_anodes_cut20MeV.png
SUM_and_individuals_anodes_cut20MeV.png
  143   Mon Jun 17 19:12:33 2019 VictorTotal SUM in coincidence with AIDA Plastic
Also TAC DTAS-Plastic AIDA
Attachment 1: Sum_coin_PlasAIDA.png
Sum_coin_PlasAIDA.png
Attachment 2: TAC_SUM_PlasAIDA.png
TAC_SUM_PlasAIDA.png
  132   Sun Jun 16 07:31:01 2019 VictorThe bump in the mutiplicities
We have calculated the spectra of the module multiplicity for each side (careful! the maximum is 8, since it is
not the total multiplicity but the multiplicity of each side).
Attachment 1: Mm_sides_1.png
Mm_sides_1.png
Attachment 2: Mm_sides_2.png
Mm_sides_2.png
Attachment 3: Mm_sides_3.png
Mm_sides_3.png
Attachment 4: Mm_sides_4.png
Mm_sides_4.png
Attachment 5: Mm_sides_5.png
Mm_sides_5.png
Attachment 6: Mm_sides_6.png
Mm_sides_6.png
Attachment 7: Mm_sides_7.png
Mm_sides_7.png
Attachment 8: Mm_sides_8.png
Mm_sides_8.png
  110   Mon Jun 10 08:07:17 2019 Ale, JoseTest of pulser count rates
File: 20190610_1602_background_AIDA_in.root

SyncPulse: 61777
DTPulser: 61277
LP_out: 61289 (!!!?)
EDy01: 61247
EDy13: 61226

LP_out counts more now
Attachment 1: 20190610_1602_background_AIDA_in.root
  142   Mon Jun 17 19:11:06 2019 VictorTAC slowest module vs fastest module DTAS
Inside events of 320ns window
Attachment 1: TAC_last_module_1st_module.png
TAC_last_module_1st_module.png
  81   Fri May 31 06:48:58 2019 A. AlgoraT spectra for AIDA and F11 plastics

T spectra for AIDAPL and F11PLL and F11PLR are defined from now on. The ancilliary card was not saving the CFD values for all channels.

It was modified in order to have those spectra. A new configuration file will be saved. See in the attachment

Attachment 1: 20190531_Conf_1.xlsx
  3   Wed May 15 04:03:23 2019 JARSynchronization with AIDA working

Synchronization with AIDA is working, see attached document to proceed.

Attachment 1: SyncProcedure.pdf
SyncProcedure.pdf
  136   Sun Jun 16 22:02:45 2019 VictorSum in coincidence with F11
TAC DTAS (slowest module of the sum) and F11

Total sum in coincidence with F11

Forward sum in coincidence with F11 (only 1-8 modules)

Backward sum in coincidence with F11 (only 11-18 modules)
Attachment 1: TAC_SUM_F11.png
TAC_SUM_F11.png
Attachment 2: Sum_coin_F11.png
Sum_coin_F11.png
Attachment 3: Sum_coin_F11_for_back.png
Sum_coin_F11_for_back.png
  6   Wed May 15 07:48:08 2019 Kiss Algora NacherSaturation 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
  42   Thu May 23 04:18:57 2019 A. AlgoraSY2527 fixed

Following the instructions of CAEN, the SY2527 is working again. Some pushing, massaging appear to solve the situation

  62   Tue May 28 05:30:03 2019 A. AlgoraReference detector threshold changed

Again the Reference detector was firing mainly in the noise. Threshold increased to 5000 !!!!

New config file was saved, rate of Ref detector now: aprox. 400 kHz

Attachment 1: Screenshot_from_2019-05-28_13-29-46.png
Screenshot_from_2019-05-28_13-29-46.png
  59   Mon May 27 12:54:48 2019 A. AlgoraReference detector

The reference detector was very noisy. The threshold has been changed from 2000 to 3200. We should look at this more carefully.

The position of the fiber was also changed. It moved too close to the Cs peak. Probably it has to do with the flexibility of the plastik screw that fixes it.

 

 

Attachment 1: Screenshot_from_2019-05-27_20-54-21.png
Screenshot_from_2019-05-27_20-54-21.png
  72   Thu May 30 02:03:33 2019 A. AlgoraRef detector position changed, AIDA plastik HV changed

The position of the reference detector in the ancilliary card was changed from channel 10 to channel 9. Remember that this is important

in relation to all files saved until now.

The HV of AIDA plastic was changed from 1300 V back to 1000 V.

A new configuration file provided by Alvaro and Jose, with some small changes will be loaded.

cp 20190529_Conf_ATJLT.xlsx 20190530_Conf.xlsx

The new configuration file has been uploaded. Reference detector appears in channel V2A8C9. It was necessary to change the range of the histogram, and to recalibrate it.

With the new configuration parameters the pulser appears at 1360 keV in the calibrated spectra of the reference detector.

The threshold of the Ref detector has also been changed. From 4400 to 2800.

Attachment 1: 20190530_Conf.xlsx
  70   Wed May 29 09:49:25 2019 A. AlgoraNew configuration file

New configuration file after a few small changes in thresholds.

Attachment 1: 20190529_Conf.xlsx
  94   Mon Jun 3 12:56:06 2019 A. AlgoraNew configuration file

The E range of the AIDA plastic for the construction of the TAIDA plastic spectrum has been changed. Also the range of the TAC_AIDAPL_CryA has been changed.

The estimated range of AIDA was based on the file 201906011624_background_AIDA_in.root, which was with no beam. But I am not sure is the calibration of 

AIDAPL is fine.

Attachment 1: 20190603_Conf.xlsx
  19   Mon May 20 06:55:15 2019 A. AlgoraNew config file after calibration

A file with Co and Cs was collected for 10 min

201905201444_137Cs60Co_align.root

after a minimal correction of the voltages (mentioned in the earlier entry). After this a new calibration was performed.

Rates per detector of the order of 1.7 kHz, Ref det rate 63 Hz, with the pulser set to 10 Hz

Now a  check on the other available sources will be performed.

Until now the used Co source was CO401(2530) , which is rather strong (corresponds to key 6)

and the Cs source was CS401 (4763) (key 8). This Cs is fine.

Now the sources on the red box (color ?) will be explored.

Configuration file: 20190520_Conf.xlsx

 

 

 

  84   Fri May 31 14:17:13 2019 A. AlgoraNew config file

A new config file provided by Jose and Alvaro is loaded

cp 20190531_Conf_JLTAT.xlsx 20190531_Conf_2.xlsx

Comments: I have modified it afterwards to have TAIDAPL, the threshold in E was too high. The TAC_F11R_CryA was also modified. It is shifted in time and cut as it was.

It remains cut.

Short root file is attached as example

---...---...---...---...---...---...---...---...---...---...---...---...---...---...---...---...---...---...---

*Update*: some of the histograms saved from DACQ online are duplicated (same name, but different cycles: ";1" and ";2"), and the second copy is empty. When you open the ROOT file and write the name of the histogram, the last copy ("cycle") is called, so the empty histogram is displayed.

$ root -l 201905312230_background_AIDA_in.root
root [0]
Attaching file 201905312230_background_AIDA_in.root as _file0...
(TFile *) 0x238ac70
root [1] ESumA->Draw() //empty!

So, there are two options: delete the second copy of the histograms, or create a newer copy of the filled histograms. In order to perform the second option, please write this line,

$ root -l 201905312230_background_AIDA_in.root
root [0]
Attaching file 201905312230_background_AIDA_in.root as _file0...
(TFile *) 0x238ac70
root [1]  for (auto&& keyAsObj : *(_file0->GetListOfKeys())){auto key = (TKey*) keyAsObj; if( 1 == key->GetCycle())_file0->Get(Form("%s;%d",key->GetName(),1))->Clone(Form("%s;%d",key->GetName(),3));  }

root [2] ESumA->Draw() //copy of ESumA;1!

The changes will not persist unless the file is opened with "update" mode and the changes are saved at the end.

Alvaro.

Attachment 1: 20190531_Conf_2.xlsx
Attachment 2: 201905312230_background_AIDA_in.root
  114   Mon Jun 10 12:31:52 2019 Ale, JoseNew calibration
New calibration with more statistics
File: 20190610_2030_60Co_137Cs_AIDA_in.root

An01_EFIR	306750	536250	606750
An02_EFIR	281250	489750	554250
An03_EFIR	282750	492750	558750
An04_EFIR	263250	456750	518250
An05_EFIR	270750	471750	534750
An06_EFIR	308250	537750	609750
An07_EFIR	290250	506250	572250
An08_EFIR	284250	494250	560250
An11_EFIR	365250	636750	720750
An12_EFIR	263250	459750	519750
An13_EFIR	321750	560250	635250
An14_EFIR	327750	572250	648750
An15_EFIR	299250	521250	590250
An16_EFIR	287250	500250	566250
An17_EFIR	296250	516750	585750
An18_EFIR	273750	479250	542250
Dy01_EFIR	34296.9	59609.4	67578.1
Dy02_EFIR	33828.1	59140.6	66953.1
Dy03_EFIR	34140.6	59453.1	67421.9
Dy04_EFIR	34140.6	59453.1	67265.6
Dy05_EFIR	34453.1	59921.9	67890.6
Dy06_EFIR	33984.4	59453.1	67421.9
Dy07_EFIR	34453.1	60078.1	68046.9
Dy08_EFIR	33828.1	58984.4	66796.9
Dy11_EFIR	34453.1	60078.1	68046.9
Dy12_EFIR	34296.9	59921.9	67890.6
Dy13_EFIR	34296.9	59609.4	67578.1
Dy14_EFIR	34296.9	59921.9	68046.9
Dy15_EFIR	33984.4	59453.1	67421.9
Dy16_EFIR	34296.9	59921.9	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	492750	558750	0.00243187	-25.7883
An04_EFIR	263250	456750	518250	0.00263384	-31.3306
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	494250	560250	0.00243187	-29.4361
An11_EFIR	365250	636750	720750	0.00188632	-27.4314
An12_EFIR	263250	459750	519750	0.00261235	-26.3813
An13_EFIR	321750	560250	635250	0.00214105	-27.0487
An14_EFIR	327750	572250	648750	0.00209042	-23.3901
An15_EFIR	299250	521250	590250	0.00230503	-28.1551
An16_EFIR	287250	500250	566250	0.00240375	-28.9034
An17_EFIR	296250	516750	585750	0.00231789	-24.9283
An18_EFIR	273750	479250	542250	0.00249619	-21.9428
Dy01_EFIR	34296.9	59609.4	67578.1	0.0201694	-29.8925
Dy02_EFIR	33828.1	59140.6	66953.1	0.0202412	-23.2189
Dy03_EFIR	34140.6	59453.1	67421.9	0.0201694	-26.741
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	33984.4	59453.1	67421.9	0.020068	-20.2545
Dy07_EFIR	34453.1	60078.1	68046.9	0.0199676	-26.3096
Dy08_EFIR	33828.1	58984.4	66796.9	0.0203445	-26.6048
Dy11_EFIR	34453.1	60078.1	68046.9	0.0199676	-26.3096
Dy12_EFIR	34296.9	59921.9	67890.6	0.0199676	-23.1897
Dy13_EFIR	34296.9	59609.4	67578.1	0.0201694	-29.8925
Dy14_EFIR	34296.9	59921.9	68046.9	0.0198974	-20.435
Dy15_EFIR	33984.4	59453.1	67421.9	0.020068	-20.2545
Dy16_EFIR	34296.9	59921.9	67578.1	0.0201077	-28.6651
Dy17_EFIR	34296.9	59921.9	67734.4	0.0200376	-25.9333
Dy18_EFIR	33984.4	59453.1	67265.6	0.020139	-23.0111
ELOG V3.1.4-unknown