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
  12   Thu May 16 02:57:15 2019 Nacher, Algorathreshold dynode #13 increased
Threshold of dynode #13 changed from 500 to 700 because of a very high noise.
New configuration file: 20190516_Conf.xlsx (attached).
Attachment 1: 20190516_Conf.xlsx
  100   Fri Jun 7 02:50:40 2019 SN, AAtest of 24Na

Start: 10:49

Stopt: 11:04

Lmd: 201906071049_24Na_AIDA_242.dlt

Root: 201906071117_24Na_AIDA_in.root

Comment: After irradiation of approximately 7 days, we extracted one Alu plate. It shows 24Na activity and also probably some beta+ activity.

The sample was not irradiated in the last 10 hours or so. It is positioned roughly in the center of the detector side in front of AIDA, using the frame prepared in Valencia.

It is not in the geometrical centre of the DTAS

Rates: 4.5 kHz (Dynodes), 4.5 (Anodes)  (Background level was at approximately 1.6-1.7 in both Dynodes, Anodes)

We need to check the alignment properly with Cs, but it looks that after one week some of the detectors have moved.

Group 1,3,5,7  (all seem to move with respect to detector 1)

Group 2,4,6,8 (detector 6 moved)

Group 11,13,15,17 (11 and 1 seem aligned, detector 13 moved)

Group 12, 14,16, 18 (12 and 2 not aligned, they seem aligned)

 

Attachment 1: 201906071117_24Na_AIDA_in.root
Attachment 2: Screenshot_from_2019-06-07_11-22-06.png
Screenshot_from_2019-06-07_11-22-06.png
Attachment 3: Screenshot_from_2019-06-07_11-24-39.png
Screenshot_from_2019-06-07_11-24-39.png
Attachment 4: Screenshot_from_2019-06-07_11-27-49.png
Screenshot_from_2019-06-07_11-27-49.png
Attachment 5: Screenshot_from_2019-06-07_11-30-17.png
Screenshot_from_2019-06-07_11-30-17.png
Attachment 6: Screenshot_from_2019-06-07_11-35-31.png
Screenshot_from_2019-06-07_11-35-31.png
Attachment 7: Screenshot_from_2019-06-07_11-36-43.png
Screenshot_from_2019-06-07_11-36-43.png
  105   Sat Jun 8 04:38:30 2019 Nacher, Algora, Tain, Molinasource top and bottom

137Cs top and bottom test... to check differences we positiones the source at the top and bottom of AIDA respectively.

Furthermore, we have changed the LED rate. Source reference: Cs401 - 4763

Root files:

201906081252_137Cs_AIDA_in_top.root  (pulser 100 Hz) (Attachment 2)

201906081228_137Cs_AIDA_in_bottom.root (pulser 10 Hz) (Attachment 3)

For each detector (An & Dy), the peak is plotted when the source is at top & bottom (Attachment 1).

 

 

Attachment 1: testOfPositioning.tar
Attachment 2: 201906081252_137Cs_AIDA_in_top.root
Attachment 3: 201906081228_137Cs_AIDA_in_bottom.root
  106   Sun Jun 9 03:59:40 2019 Manysome 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.

  120   Sat Jun 15 18:15:08 2019 Pancho& Kikerun 9
Shifters: Pancho & Kike

Degrader: none
Comments :
Last configuration file: 190615_1935_Conf_DTAS.xlsx
########################################################

Date: 2019-06-16
Start: 00:35
DTAS run: 009
AIDA run: _26
BigRIPS run: 2006

Listmode DLT: 190616_0035_100Sn_009.dlt


########################################################
----> TODO LIST during shift (check it!)<----
CHECK HISTOGRAMS/ Time: xxxx
LSUMA (hist. 3), LSUMD (hist. 4), LCryA (hist. 7), LCryD (hist. 8) - OK
F11PLR (and *L) (hist. 65 and 66) - OK
AIDAPL (hist. 69) - OK
ERefAn (hist. 70) - OK
Group Dynodes, Anodes, Ancilliaries - OK
*****************

DTAS Rate-dynodes: 3.8kHz
DTAS Rate-anodes: 3.3kHz
F11 Rate (hist. 27 or 28): 180 cps
AIDA Veto Plastic Rate (hist. 26): 13 cps

Beam current: 6965 enA (134 pnA, = enA/Zet(Xe), Zet(Xe)=52)

************************************************************************************

************************************************************************************



########################################################

Date: June-16th
Stop:
DTAS run:
AIDA run:
BigRIPS run:

Online ROOT file:

########################################################

Note:

Images:

Image entitled EDy01 corresponds to Energy of Crystal Dynod 01 (black) and 11 (red)
Image entitled EDy02 corresponds to Energy of Crystal Dynod 02 (black) and 12 (red)
Image entitled EDy03 corresponds to Energy of Crystal Dynod 03 (black) and 13 (red) .. and so on

Image entitled ECryA corresponnd to the sum of anode signal of all crystals (black) and the TAS sum (red)
Attachment 1: Screenshot_from_2019-06-16_01-50-05.png
Screenshot_from_2019-06-16_01-50-05.png
Attachment 2: Screenshot_from_2019-06-16_01-50-40.png
Screenshot_from_2019-06-16_01-50-40.png
Attachment 3: Screenshot_from_2019-06-16_01-51-11.png
Screenshot_from_2019-06-16_01-51-11.png
Attachment 4: Screenshot_from_2019-06-16_01-51-35.png
Screenshot_from_2019-06-16_01-51-35.png
Attachment 5: Screenshot_from_2019-06-16_01-52-10.png
Screenshot_from_2019-06-16_01-52-10.png
Attachment 6: Screenshot_from_2019-06-16_01-52-37.png
Screenshot_from_2019-06-16_01-52-37.png
Attachment 7: Screenshot_from_2019-06-16_01-53-01.png
Screenshot_from_2019-06-16_01-53-01.png
Attachment 8: Screenshot_from_2019-06-16_01-53-35.png
Screenshot_from_2019-06-16_01-53-35.png
Attachment 9: Screenshot_from_2019-06-16_01-47-11.png
Screenshot_from_2019-06-16_01-47-11.png
  121   Sat Jun 15 18:38:15 2019 Pancho & Kikerun 12
Shifters: Pancho & Kike

Degrader: none
Comments :
Last configuration file: 190615_1935_Conf_DTAS.xlsx
########################################################

Date: 2019-06-16
Start: 02:33
DTAS run: 012
AIDA run: 43
BigRIPS run: 2007

Listmode DLT: 190616_0233_100Sn_012.dlt



########################################################
----> TODO LIST during shift (check it!)<----
CHECK HISTOGRAMS/ Time: xxxx
LSUMA (hist. 3), LSUMD (hist. 4), LCryA (hist. 7), LCryD (hist. 8) - OK
F11PLR (and *L) (hist. 65 and 66) - OK
AIDAPL (hist. 69) - OK
ERefAn (hist. 70) - OK
Group Dynodes, Anodes, Ancilliaries - OK
*****************

DTAS Rate-dynodes: 4.0kHz
DTAS Rate-anodes: 3.3kHz
F11 Rate (hist. 27 or 28): 180 cps
AIDA Veto Plastic Rate (hist. 26): 12 cps

Beam current: 6886 enA (132 pnA, = enA/Zet(Xe), Zet(Xe)=52)

************************************************************************************

************************************************************************************



########################################################

Date: June-16th
Stop:
DTAS run:
AIDA run:
BigRIPS run:

Online ROOT file:
########################################################

Note:
  133   Sun Jun 16 19:18:15 2019 Ela, Victorroot 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
  122   Sat Jun 15 18:39:07 2019 Pancho & Kikeroot files
100Sn root files corresponding to runs 06,07,08 (190616_0030_100Sn_008.root) and runs 09,10,11 (190616_0230_100Sn_011.root) two hours each
Attachment 1: 190616_0030_100Sn_008.root
Attachment 2: 190616_0230_100Sn_011.root
  8   Wed May 15 09:57:54 2019 Nacherroot file with 60Co and 137Cs

For JL to play...

Attachment 1: 201905151432_137Cs60Co.root
  124   Sat Jun 15 22:43:20 2019 Pancho & Kikeroot file data 4:30 - 6:30
corresponding to runs .dlt 15-17


Images:

EAn01: All anodes energies overlay. EAn12 shows a bump between 50-100 keV and a peak between 100-120 keV


LAn01: all anodes lights overlayed. In LAn06 a peak is seen between 20-30 au (keV?); for LAn12 two bumps are seen between 80-120 au (keV?) and between 130-150 au (keV?)
Attachment 1: 190616_0630_100Sn_017.root
Attachment 2: Screenshot_from_2019-06-16_06-41-32.png
Screenshot_from_2019-06-16_06-41-32.png
Attachment 3: Screenshot_from_2019-06-16_06-42-55.png
Screenshot_from_2019-06-16_06-42-55.png
  123   Sat Jun 15 20:43:50 2019 Pancho & Kikeroot file data 2:30 - 4:30
corresponding to runs .dlt 12-14
Attachment 1: 190616_0430_100Sn_014.root
  128   Sun Jun 16 03:42:17 2019 Ela, Sonja, Victorroot file 8:30-10:30
Attachment 1: 190616_1032_100Sn_023.root
  125   Sun Jun 16 00:52:27 2019 Ela, Sonja, Victorroot file 6:30-8:30
Attachment 1: 190616_0833_100Sn_020.root
  139   Sun Jun 16 23:37:47 2019 Ela, Victorroot file 5:30-7:30
Attachment 1: 190617_0730_100Sn_054.root
  135   Sun Jun 16 21:44:38 2019 Ela, Victorroot file 3:30-5:30
Attachment 1: 190617_0528_100Sn_051.root
  138   Sun Jun 16 23:37:18 2019 Ela, Victorroot file 3:30-5:30
Attachment 1: 190617_0528_100Sn_051.root
  134   Sun Jun 16 21:43:36 2019 Ela, Victorroot file 1:30-3:30
Attachment 1: 190617_0325_100Sn_048.root
  130   Sun Jun 16 06:55:31 2019 Ela, Sonja, Victorroot file 12:30-14:30
Attachment 1: 190616_1435_100Sn_029.root
  129   Sun Jun 16 04:44:05 2019 Ela, Sonja, Victorroot file 10:30-12:30
The beam stopped a couple of times due to problems before RRC
Attachment 1: 190616_1233_100Sn_026.root
Attachment 2: Runs_24-26_breaks.png
Runs_24-26_breaks.png
  137   Sun Jun 16 22:56:41 2019 Victorrates modules in coincidence with F11
Module	Rate cps	Rate coin. F11 cps	Difference cps
1	36.8868		13.4045			23.4824
2	11.9046		1.16338			10.7412
3	35.5992		12.8111			22.7881
4	12.114		1.2723			10.8417
5	37.6139		13.2296			24.3843
6	12.793		1.33943			11.4536
7	37.7954		13.4383			24.3571
8	12.4813		1.3365			11.1448
11	29.6067		7.84707			21.7597
12	12.0162		0.859941		11.1563
13	28.9357		7.5685			21.3672
14	11.4407		0.825287		10.6154
15	29.7828		7.77872			22.0041
16	11.4512		0.847232		10.604
17	29.7826		8.0374			21.7452
18	11.3122		0.850505		10.4617
  131   Sun Jun 16 07:08:10 2019 Ela, Sonja, Victor, Alejandroproblems 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
Crystals_coincidence_F11.png
Attachment 2: TAC_crystals_coincidence_F11.png
TAC_crystals_coincidence_F11.png
  60   Mon May 27 13:50:54 2019 A. Algorapreparation directory moved

The preparation directory was moved to /data/DRikenPreparation (from its first place /home/dacq/DRikenPreparation) because the lack of space.

  98   Thu Jun 6 09:36:52 2019 Alvaro, Jorge, Alenew config file
New config file: 20190606_Conf.xlsx

Changed with respect to the earlier file (20190605_Conf.xlsx):

-The threshold of the Reference detector was changed from 2800 to 3500.
-A new gated histogram was added: ECryA gated by F11PLR in the energy range of the implanted ions, named as
EcryAGF11

Issue in AIDA PL (see screenshot). A lot of small signals; top, samples, bottom output of EFIR (picture taken
when integration = 50 samples; value in configuration = 20)
Attachment 1: 20190606_Conf.xlsx
Attachment 2: Screenshot_from_2019-06-06_16-54-15.png
Screenshot_from_2019-06-06_16-54-15.png
  99   Fri Jun 7 01:55:24 2019 CA, JA , ATmerger test
Setup: On 17th-May (11:18 - 11:38), AIDA was inside DTAS. Measurement of 60Co source.

Files:
AIDA: R6_{3..7}.gz
1,2G may 17 11:21 R6_3.gz
982M may 17 11:25 R6_4.gz
926M may 17 11:28 R6_5.gz
1,1G may 17 11:32 R6_6.gz
1,2G may 17 11:38 R6_7.gz
 20M may 17 11:39 R6_8.gz

DTAS: AidaMergerTest_2_0{23..29}.dlt
955M may 17 11:21 AidaMergerTest_2_023.dlt
955M may 17 11:24 AidaMergerTest_2_024.dlt
956M may 17 11:27 AidaMergerTest_2_025.dlt
956M may 17 11:31 AidaMergerTest_2_026.dlt
955M may 17 11:33 AidaMergerTest_2_027.dlt
956M may 17 11:36 AidaMergerTest_2_028.dlt
732M may 17 11:38 AidaMergerTest_2_029.dlt


Working dir: ~/Corrigan

Test 1: merge R6_5 with AidaMergerTest_2_025.dlt
  68   Wed May 29 08:29:26 2019 A. Algoralatest conf file

Latest configuration file from 28 of May

Attachment 1: 20190528_Conf.xlsx
  28   Tue May 21 06:44:18 2019 A. Algoraidentified useful sources

This is a short list of the identified useful sources:

60Co, key 3, red box, CD 395, already used

137Cs, key 8, 4753, CS401, activity ???, already used

22Na, key 5, 700, NA401, activity 8.9 kBq/s

152Eu, key 9, 272, EU401, activity 6.6 kBq/s

The activities are according to the Sunflower homepage. It was wrong for the Cs source which is under key 8

  18   Mon May 20 06:31:53 2019 A. Algoragain correction

Only a very small correction was needed (at the level of 0.5 V) for the raw spectra of det 6,12,13,17 (raw Dynodes)

New voltages

DET01        │ 599.0 V 1500.0 uA  598.5 V   89.5 uA On                 │00.0001
DET02        │ 548.5 V 1500.0 uA  548.0 V   82.5 uA On                 │00.0002
DET03        │ 529.0 V 1500.0 uA  529.0 V   79.5 uA On                 │00.0003
DET04        │ 699.0 V 1500.0 uA  698.5 V  105.0 uA On                 │00.0004
DET05        │ 452.0 V 1500.0 uA  451.5 V   67.5 uA On                 │00.0005
DET06        │ 820.5 V 1500.0 uA  821.0 V  123.0 uA On                 │00.0006
DET07        │ 559.0 V 1500.0 uA  559.0 V   83.0 uA On                 │00.0007
DET08        │ 486.0 V 1500.0 uA  486.0 V   73.0 uA On                 │00.0008
EMPTY09      │   0.0 V 1500.0 uA    1.0 V    7.5 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        │ 578.0 V  300.0 uA  578.0 V   86.5 uA On                 │02.0001
DET12        │505.5  V  300.0 uA  506.0 V   76.0 uA On                 │02.0002
DET13        │ 624.5 V  300.0 uA  624.5 V   92.5 uA On                 │02.0003
DET14        │ 650.0 V  300.0 uA  650.0 V   96.0 uA On                 │02.0004
DET15        │ 657.0 V  300.0 uA  657.0 V   98.0 uA On                 │02.0005
DET16        │ 529.5 V  300.0 uA  529.0 V   78.5 uA On                 │00.0006
DET17        │ 462.5 V  300.0 uA  462.0 V   68.0 uA On                 │00.0007
DET18        │ 518.0 V  300.0 uA  518.0 V   77.5 uA On                 │00.0008
EMPTY19      │   0.0 V  300.0 uA    0.0 V    0.0 uA Off                │00.0009
EMPTY20      │   0.0 V  300.0 uA    0.0 V    0.0 uA Off                │00.0010
REF01        │ 800.0 V 1500.0 uA  800.0 V  174.0 uA On                 │00.0011
EMPTY12      │   0.0 V 1500.0 uA    0.0 V    0.0 uA Off                │02.0000

 

 

  15   Sat May 18 01:41:45 2019 Nacher, Algoragain 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

  107   Sun Jun 9 04:03:38 2019 Jorge, Jose, Pancho, Alvaro, Kike, Aleeffect 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
Screenshot_from_2019-06-09_14-27-37.png
Attachment 2: Screenshot_from_2019-06-09_14-31-32.png
Screenshot_from_2019-06-09_14-31-32.png
  53   Mon May 27 07:11:22 2019 A. Algoradetectors realigned with Cs

Small alignment corrections were needed, of the order of 0.5-1V.

All detectors were realigned

Attachment 1: Screenshot_from_2019-05-27_15-13-09.png
Screenshot_from_2019-05-27_15-13-09.png
  11   Thu May 16 02:02:24 2019 Algora Kiss Nacherdetector 3 moved over night
After the long background measurement we have measured 60Co to check alignment.
Everything looks fine except for detector #3 that has moved to lower gain (seen in dynodes and anodes).
See figures attached.
Attachment 1: Screenshot_from_2019-05-16_10-00-53.png
Screenshot_from_2019-05-16_10-00-53.png
Attachment 2: Screenshot_from_2019-05-16_10-01-29.png
Screenshot_from_2019-05-16_10-01-29.png
Attachment 3: Screenshot_from_2019-05-16_10-01-57.png
Screenshot_from_2019-05-16_10-01-57.png
Attachment 4: Screenshot_from_2019-05-16_10-09-16.png
Screenshot_from_2019-05-16_10-09-16.png
  79   Thu May 30 12:08:01 2019 A. Algorabackground, dacq restarted before the measurement

Start: 20:09

Stop: 10:17

Root:  201905311017_background_AIDA_in.root

Comments: before this measurement  the system was restarted.

LED in EDy16 looks wider

The TACS were recovered. Probably all the files of today (until now) and generated after the configuration file change do not have the calibrated spectra.

Attachment 1: 201905311017_background_AIDA_in.root
Attachment 2: 20190530_Conf.xlsx
  116   Mon Jun 10 13:02:16 2019 Jose, Pancho, Alebackground, 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
  45   Fri May 24 08:33:52 2019 A. Algorabackground, AIDA is out

Start: 16:35

Stop: 17:30

Rates: 1.5 kHz (Dynodes), 1.8 kHz (Anodes)

Listmode: Background_201905241635_082.dlt ...Background_201905241635_086.dlt

Root: 201905241730_background.root

Attachment 1: 201905241730_background.root
  34   Tue May 21 12:04:10 2019 A. Algorabackground without listmode

Start: 20:04

Stop: 14:11

Rates: 1.8 (Dynodes) 2.0 kHz (anodes)

Attachment 1: 201905221411_background.root
  97   Tue Jun 4 06:27:55 2019 A. Algora (++Jorge,++ Alvaro)background with no beam

Start: 14:25

Stop: 14:39 (partial, no beam, not erased), 14:58 (partial, no beam, not erased), 15:16  (partial, no beam, not erased),

Stop: 14:39 (next day, a new spectrum was added, AIDAGF11)

Root: 201906041439_background_AIDA_in.root, 201906041458_background_AIDA_in.root, 201906041516_background_AIDA_in.root

 

Comment: They enter to change the F3, F7 plastics. So the beam was stopped.

Beam from approximately 15:25, syncronization pulse was sent. Rate at F7 9.4 kHz

Attachment 1: 201906041439_background_AIDA_in.root
Attachment 2: 201906041458_background_AIDA_in.root
Attachment 3: 201906041516_background_AIDA_in.root
Attachment 4: 201906051343_background_AIDA_in.root
Attachment 5: 201906051439_background_AIDA_in.root
  88   Sat Jun 1 10:04:54 2019 A. Algorabackground with beam

Start: 18:05

Stop: 22:27

Comments: Rate at F7: 3,3 kHz, rate at F11 (according to the in-beam team approx. 2.4 kHz)

Root: 201906012227_background_AIDA_in.root

In the graph: F11PL R and L, below Aida pl, below TCryA

Attachment 1: 201906012227_background_AIDA_in.root
Attachment 2: Screenshot_from_2019-06-01_22-29-51.png
Screenshot_from_2019-06-01_22-29-51.png
  118   Wed Jun 12 02:04:07 2019 AA, EN, PM, ATbackground during in-beam exp.
In-beam experiment going on. Only 12h of beam in the last 21h.

Start: ~1pm (11th-June)
Stop: ~10am (12th-June)
Attachment 1: 20190612_0959_background_AIDA_in.root
  21   Mon May 20 08:15:24 2019 A. Algorabackground

Start: 16:25

Stop: 17:25

Background in the same conditions as before (right after the Co measurement)

Listmode: Background_201905201614_035.dlt .... Background_201905201614_036.dlt

Root file:  201905201725_background.root

Rates:

Dynodes: 8.5 kHz

Anodes: 1.8 kHz

Anod1: 120 Hz

Anod15: 173 Hz

Dynod1: 80 Hz

Dynod 15: 166 Hz

Pulser set to 10 Hz

Rate of Dynode 5, 15, 17  seem a little higher than the others. The same for Anode 11, 15, 17

Not clear why the Dynodes rate is so high compared with the anodes. There is not such a big

difference in rate of the individual detectors.  

(Dynodes and Anodes rates are taken from the Python script written by Jorge, that correspond to the full card)

Later it become evident that probably we need to increase  the threshold of detector 8 again (Dy08).

Before it was not like that, but now seems to be triggering in the noise.

 

 

Attachment 1: Screenshot_from_2019-05-20_16-43-50.png
Screenshot_from_2019-05-20_16-43-50.png
Attachment 2: Screenshot_from_2019-05-20_16-45-46.png
Screenshot_from_2019-05-20_16-45-46.png
Attachment 3: 201905201725_background.root
  24   Mon May 20 12:29:05 2019 A. Algorabackground

Start: 20:30

Stop: 09:54

Lmd: Background_201905202030_046.dlt ...Background_201905202030_051.dlt

Root: 201905210954_background.root

 

Root and Conf file attached

Attachment 1: 201905210954_background.root
Attachment 2: 20190520_Conf_3.xlsx
  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
  109   Mon Jun 10 04:18:24 2019 Ale, JoseNew Configuration File
File:  20190610_1145_Conf_DTAS.xlsx

Several changes and corrections
Naming: V2A8C1 -> Aux01, ...

New or corrected
Aux13 -> LP_out (puse out of light pulser)
Aux15 -> DTpulser (Out of GSI clock triggering LP)
Aux16 -> SyncPulser (Out of GSI clock send out for synchronization with AIDA & BigRIPS)

Ranges changed
Aux09, ERefAn

We observed that LP_out was counting less than the other two
so we tried to check DACQ parameters. We basically change nothing
Only activated "CFD time"
Note that pulse out is a very strange signal:
Negative(?),-400mV offset, 200mV high
In the DACQ is treated as positive signal with a large negative offset.
Attachment 1: 20190610_1145_Conf_DTAS.xlsx
  115   Mon Jun 10 12:48:01 2019 Ale, JoseNew Config file
Conf file with new calibration:
20190610_2035_Conf_DTAS.xlsx

Check root file:
20190610_2050_60Co_137Cs_AIDA_in.root

See screen shots:
Attachment 1: 20190610_2035_Conf_DTAS.xlsx
Attachment 2: 20190610_2050_60Co_137Cs_AIDA_in.root
Attachment 3: Screenshot_from_2019-06-10_20-54-43.png
Screenshot_from_2019-06-10_20-54-43.png
Attachment 4: Screenshot_from_2019-06-10_20-55-42.png
Screenshot_from_2019-06-10_20-55-42.png
Attachment 5: Screenshot_from_2019-06-10_20-56-39.png
Screenshot_from_2019-06-10_20-56-39.png
Attachment 6: Screenshot_from_2019-06-10_20-57-29.png
Screenshot_from_2019-06-10_20-57-29.png
  113   Mon Jun 10 10:44:36 2019 Ale, JoseNew Conf file with new calibration
File: 20190610_1835_Conf_DTAS.xlsx
  126   Sun Jun 16 01:36:08 2019 VictorMm 100Sn beam
Attachment 1: Mm_beam_ON_100Sn_runs9-11.png
Mm_beam_ON_100Sn_runs9-11.png
Attachment 2: Mm_beam_ON_100Sn_runs9-11_zoom.png
Mm_beam_ON_100Sn_runs9-11_zoom.png
Attachment 3: Mm_beam_ON_100Sn_runs9-11.C
{
//=========Macro generated from canvas: c2/Canvas
//=========  (Sun Jun 16 02:44:48 2019) by ROOT version5.34/36
   TCanvas *c2 = new TCanvas("c2", "Canvas",65,24,1303,744);
   gStyle->SetOptStat(0);
   c2->Range(0,0,1,1);
   c2->SetFillColor(10);
   c2->SetBorderMode(0);
   c2->SetBorderSize(2);
   c2->SetFrameFillColor(0);
   c2->SetFrameBorderMode(0);
  
// ------------>Primitives in pad: pad1
   TPad *pad1 = new TPad("pad1", "Pad",0,0,1,1);
   pad1->Draw();
   pad1->cd();
   pad1->Range(-594.2857,-23200.36,4361.905,120612);
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   pad1->SetBorderMode(0);
   pad1->SetBorderSize(2);
   pad1->SetLeftMargin(0.1199078);
   pad1->SetRightMargin(0.04073789);
   pad1->SetTopMargin(0.07777778);
   pad1->SetBottomMargin(0.1402778);
   pad1->SetFrameFillColor(0);
   pad1->SetFrameBorderMode(0);
   pad1->SetFrameBorderMode(0);
   
   TH1D *E_SUM = new TH1D("E_SUM"," ",14000,0,140000);
   E_SUM->SetBinContent(2,105345);
   E_SUM->SetBinContent(3,95898);
   E_SUM->SetBinContent(4,46529);
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   E_SUM->SetBinContent(21,117725);
   E_SUM->SetBinContent(22,116024);
   E_SUM->SetBinContent(23,118288);
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   E_SUM->SetBinContent(157,22251);
   E_SUM->SetBinContent(158,19958);
   E_SUM->SetBinContent(159,18371);
   E_SUM->SetBinContent(160,17047);
   E_SUM->SetBinContent(161,16007);
   E_SUM->SetBinContent(162,15355);
   E_SUM->SetBinContent(163,15208);
   E_SUM->SetBinContent(164,15380);
   E_SUM->SetBinContent(165,15338);
   E_SUM->SetBinContent(166,15968);
   E_SUM->SetBinContent(167,15840);
   E_SUM->SetBinContent(168,15969);
   E_SUM->SetBinContent(169,15595);
   E_SUM->SetBinContent(170,15237);
   E_SUM->SetBinContent(171,14957);
   E_SUM->SetBinContent(172,14235);
   E_SUM->SetBinContent(173,14081);
   E_SUM->SetBinContent(174,13541);
   E_SUM->SetBinContent(175,13582);
   E_SUM->SetBinContent(176,13532);
   E_SUM->SetBinContent(177,13609);
   E_SUM->SetBinContent(178,13965);
   E_SUM->SetBinContent(179,13724);
   E_SUM->SetBinContent(180,13610);
   E_SUM->SetBinContent(181,13617);
   E_SUM->SetBinContent(182,12797);
   E_SUM->SetBinContent(183,12357);
   E_SUM->SetBinContent(184,11878);
   E_SUM->SetBinContent(185,11269);
   E_SUM->SetBinContent(186,10773);
   E_SUM->SetBinContent(187,10407);
   E_SUM->SetBinContent(188,10348);
   E_SUM->SetBinContent(189,10151);
   E_SUM->SetBinContent(190,9992);
   E_SUM->SetBinContent(191,10065);
   E_SUM->SetBinContent(192,10345);
   E_SUM->SetBinContent(193,10721);
   E_SUM->SetBinContent(194,10970);
   E_SUM->SetBinContent(195,11589);
   E_SUM->SetBinContent(196,12053);
   E_SUM->SetBinContent(197,11978);
   E_SUM->SetBinContent(198,12575);
   E_SUM->SetBinContent(199,12476);
   E_SUM->SetBinContent(200,12122);
   E_SUM->SetBinContent(201,11362);
   E_SUM->SetBinContent(202,11014);
   E_SUM->SetBinContent(203,10344);
   E_SUM->SetBinContent(204,9735);
   E_SUM->SetBinContent(205,9402);
   E_SUM->SetBinContent(206,9199);
   E_SUM->SetBinContent(207,8557);
   E_SUM->SetBinContent(208,8106);
   E_SUM->SetBinContent(209,8040);
   E_SUM->SetBinContent(210,7840);
   E_SUM->SetBinContent(211,7486);
   E_SUM->SetBinContent(212,7471);
   E_SUM->SetBinContent(213,7414);
   E_SUM->SetBinContent(214,7468);
   E_SUM->SetBinContent(215,7534);
   E_SUM->SetBinContent(216,7484);
   E_SUM->SetBinContent(217,7685);
   E_SUM->SetBinContent(218,7718);
   E_SUM->SetBinContent(219,7916);
   E_SUM->SetBinContent(220,7880);
   E_SUM->SetBinContent(221,7868);
   E_SUM->SetBinContent(222,7807);
   E_SUM->SetBinContent(223,8064);
   E_SUM->SetBinContent(224,7881);
   E_SUM->SetBinContent(225,7774);
   E_SUM->SetBinContent(226,7751);
   E_SUM->SetBinContent(227,7434);
   E_SUM->SetBinContent(228,7479);
   E_SUM->SetBinContent(229,7235);
   E_SUM->SetBinContent(230,7044);
   E_SUM->SetBinContent(231,7044);
   E_SUM->SetBinContent(232,7016);
   E_SUM->SetBinContent(233,7003);
   E_SUM->SetBinContent(234,7093);
   E_SUM->SetBinContent(235,6902);
   E_SUM->SetBinContent(236,6962);
   E_SUM->SetBinContent(237,6880);
   E_SUM->SetBinContent(238,6865);
   E_SUM->SetBinContent(239,7001);
   E_SUM->SetBinContent(240,6883);
   E_SUM->SetBinContent(241,6953);
   E_SUM->SetBinContent(242,6866);
   E_SUM->SetBinContent(243,7012);
   E_SUM->SetBinContent(244,7290);
   E_SUM->SetBinContent(245,7296);
   E_SUM->SetBinContent(246,7356);
   E_SUM->SetBinContent(247,7568);
   E_SUM->SetBinContent(248,7612);
   E_SUM->SetBinContent(249,7569);
   E_SUM->SetBinContent(250,7653);
   E_SUM->SetBinContent(251,7571);
   E_SUM->SetBinContent(252,7552);
   E_SUM->SetBinContent(253,7499);
   E_SUM->SetBinContent(254,7481);
   E_SUM->SetBinContent(255,7500);
   E_SUM->SetBinContent(256,7456);
   E_SUM->SetBinContent(257,7588);
   E_SUM->SetBinContent(258,7308);
   E_SUM->SetBinContent(259,7741);
   E_SUM->SetBinContent(260,7906);
   E_SUM->SetBinContent(261,7926);
   E_SUM->SetBinContent(262,8243);
   E_SUM->SetBinContent(263,8322);
   E_SUM->SetBinContent(264,8371);
   E_SUM->SetBinContent(265,8466);
   E_SUM->SetBinContent(266,8582);
   E_SUM->SetBinContent(267,8565);
   E_SUM->SetBinContent(268,8424);
   E_SUM->SetBinContent(269,8337);
   E_SUM->SetBinContent(270,8008);
   E_SUM->SetBinContent(271,7815);
   E_SUM->SetBinContent(272,7640);
... 20627 more lines ...
Attachment 4: Mm_beam_ON_100Sn_runs9-11_linear.png
Mm_beam_ON_100Sn_runs9-11_linear.png
  141   Mon Jun 17 06:28:06 2019 VictorMC number of implants
           Counts in DTAS
Proposal   2730 
4 days     888
5 days     1102
10 days    2196
Attachment 1: MC_100Sn_days.png
MC_100Sn_days.png
  96   Tue Jun 4 06:25:51 2019 A. AlgoraLead shielding was "upgraded"

With the help of Tom the additional lead pieces were put. So now the hole in the lead shielding matches the hole in the polyethylene shielding.

The hole is 11 cm x 11 cm approximately

 

  44   Fri May 24 07:57:51 2019 A. AlgoraLead shielding heigth increased

The aluminium plate of 3 cm thickness arrived and the lead shielding was dismounted and mounted again. We left a narrower hole in it.

Special thanks to Tom, who helped with the hard physical work.

  66   Wed May 29 02:07:20 2019 A. AlgoraIrradiation for 24Na

Irradiation of two pieces of aluminium of 80 mm x 40 mm x 10 mm will be performed at the second BigRips dipole.

The pieces were placed with the help of Fukuda and Nishimura san.

  2   Tue May 14 13:16:33 2019 JLTHardware setup
Attachment 1: DTAS-setup.png
DTAS-setup.png
Attachment 2: DTAS-shielding.pdf
DTAS-shielding.pdf
Attachment 3: InnerSuportFrame.pdf
InnerSuportFrame.pdf
Attachment 4: DTAS-assembly.png
DTAS-assembly.png
Attachment 5: DTAS-module.png
DTAS-module.png
Attachment 6: DTAS-PMT.pdf
DTAS-PMT.pdf DTAS-PMT.pdf
Attachment 7: DTAS-VD.pdf
DTAS-VD.pdf
Attachment 8: WellDetector.png
WellDetector.png
Attachment 9: WellDetector-PMT.pdf
WellDetector-PMT.pdf WellDetector-PMT.pdf
Attachment 10: MSI-8-P.pdf
MSI-8-P.pdf MSI-8-P.pdf MSI-8-P.pdf MSI-8-P.pdf MSI-8-P.pdf MSI-8-P.pdf MSI-8-P.pdf MSI-8-P.pdf MSI-8-P.pdf MSI-8-P.pdf
Attachment 11: 6010_datasheet.pdf
6010_datasheet.pdf 6010_datasheet.pdf
  56   Mon May 27 07:34:58 2019 A. AlgoraHV status

EMPTY00    │   0.0 V 1500.0 uA    0.5 V    0.5 uA Off                │00.0000
DET01        │ 599.0 V 1500.0 uA  598.5 V   90.0 uA On                 │00.0001
DET02        │ 548.5 V 1500.0 uA  548.0 V   82.5 uA On                 │00.0002
DET03        │ 530.5 V 1500.0 uA  530.0 V   80.0 uA On                 │00.0003
DET04        │ 697.5 V 1500.0 uA  697.5 V  105.0 uA On                    Admi4
DET05        │ 451.5 V 1500.0 uA  451.0 V   67.5 uA On                       05
DET06        │ 820.0 V 1500.0 uA  820.5 V  123.0 uA On  Status             Ch06
DET07        │ 560.0──────────────560.0 V   84.0 uA On ────────────────┬─0.0007
DET08        │ 486.0 V 1500.0 uA  486.0 V   73.0 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                │00.0000
DET11        │ 579.0 V  300.0 uA  579.5 V   86.5 uA On                 │00.0001
DET12        │ 506.0 V  300.0 uA  506.5 V   76.0 uA On                 │00.0002
DET13        │ 623.5 V  300.0 uA  623.5 V   92.5 uA On                 │00.0003
DET14        │ 649.5 V  300.0 uA  649.5 V   96.5 uA On                 │00.0004
DET15        │ 656.5 V  300.0 uA  656.5 V   97.5 uA On                 │00.0005
DET16        │ 530.5 V  300.0 uA  530.0 V   78.5 uA On                 │00.0006
EMPTY12    │   0.0 V 1500.0 uA    0.0 V    0.0 uA Off                │02.0000
DET11        │ 578.0 V  300.0 uA  578.0 V   86.5 uA On                 │02.0001
DET12        │505.5  V  300.0 uA  506.0 V   76.0 uA On                 │02.0002
DET13        │ 624.5 V  300.0 uA  624.5 V   92.5 uA On                 │02.0003
DET14        │ 650.0 V  300.0 uA  650.0 V   96.0 uA On                 │02.0004
DET15        │ 657.0 V  300.0 uA  657.0 V   98.0 uA On                 │02.0

DET16        │ 530.5 V  300.0 uA  530.0 V   78.5 uA On                 │00.0006
DET17        │ 462.0 V  300.0 uA  461.5 V   68.0 uA On                 │00.0007
DET18        │ 518.5 V  300.0 uA  518.5 V   77.5 uA On                 │00.0008
EMPTY19    │   0.0 V  300.0 uA    0.0 V    0.0 uA Off                │00.0009
EMPTY20    │   0.0 V  300.0 uA    0.0 V    0.0 uA Off                │00.0010
REF01        │ 800.0 V  300.0 uA  800.0 V  174.0 uA On                 │00.0011
EMPTY12    │   0.0 V 1500.0 uA    0.0 V    0.0 uA Off                │02.0000

 

  5   Wed May 15 06:53:52 2019 Nacher Kiss AlgoraHV 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

 

  111   Mon Jun 10 09:58:42 2019 Jose, AleGain 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
Screenshot_from_2019-06-10_17-58-00.png
Attachment 2: Screenshot_from_2019-06-10_17-57-56.png
Screenshot_from_2019-06-10_17-57-56.png
  67   Wed May 29 07:04:19 2019 A. AlgoraF11 plastic connected

F11 plastic has been connected to our dacq as it was in the earlier BRIKEN setting.

The detector cables were followed and connections checked.

The outputs of the detector (L and R) go through an Ortec TFA 474 with the following settings:

Coarse gain: x4

Fine gain: looks minimal

Integrate (ns): 200

Diff (ns): 100

Non-inv setting

After the TFA, the Right signal is plugged in channel 1 of our card, and an attenuated signal (50 Ohm) is

plugged in channel 3. Similarly the Left signal after the TFA is plugged in channel 2 and the attenuated 

signal is plugged in channel 4.


Parameters of the channels of the dacq have to be checked.

  7   Wed May 15 08:11:46 2019 Tolosa, Nacher, Algora, KissEnergy resolutions
Using getSigmaCal.cxx macro to check energy resolutions...
root [3] getSigmaCal("201905151555_137Cs.root")


EAn01	660.978	20.4516	7.27122%	

EAn02	662.018	21.8206	7.74577%	

EAn03	654.685	21.2331	7.62164%	

EAn04	664.496	21.7799	7.70251%	

EAn05	661.188	21.3019	7.57112%	

EAn06	663.225	22.609	8.01103%	

EAn07	658.977	21.7486	7.75584%	

EAn08	661.333	21.1595	7.51887%	

EAn11	660.622	20.6158	7.33354%	

EAn12	662.106	22.8196	8.09931%	

EAn13	660.16	19.4654	6.92918%	

EAn14	660.348	22.9705	8.17459%	

EAn15	660.277	19.6762	7.00298%	

EAn16	661.323	22.0482	7.83478%	

EAn17	659.072	21.5303	7.6769%	

EAn18	662.739	22.9924	8.15284%	

EDy01	660.951	20.8514	7.41366%	

EDy02	661.465	22.2272	7.89669%	

EDy03	654.887	21.7742	7.81345%	

EDy04	663.585	22.2593	7.88284%	

EDy05	660.353	21.7962	7.75661%	

EDy06	661.692	23.2316	8.25072%	***

EDy07	658.636	22.3986	7.99178%	

EDy08	662.167	21.8422	7.75169%	

EDy11	661.634	21.2086	7.53289%	

EDy12	662.504	23.1784	8.22173%	***

EDy13	660.297	20.7076	7.36985%	

EDy14	662.493	23.5084	8.33893%	***

EDy15	661.844	20.3493	7.22539%	

EDy16	662.861	23.092	8.18665%	

EDy17	661.152	22.215	7.89612%	

EDy18	659.903	23.6411	8.41889%	***
Attachment 1: getSigmaCal.cxx
#include "TH1.h"
#include "TSpectrum.h"
#include "TFile.h"
#include "TGraph.h"
#include "TF1.h"
#include "TMath.h"

#include <string>
#include <cmath>
#include <vector>
#include <iostream>
#include <map>
#include <sstream>


constexpr int eblow = 10; //bins
constexpr int rebinFac = 1; //
constexpr int maxnpeaks = 10; //max peaks to look for
constexpr double sigmaPeak = 4.0;
constexpr double thrPeak = 0.05;

constexpr double ene60Co1 = 1173.2;// keV
constexpr double ene60Co2 = 1332.5;// keV
constexpr double ene137Cs = 661.66;// keV

const std::vector<std::string> histoNames_v = { "EAn01",
						"EAn02",
						"EAn03",
						"EAn04",
						"EAn05",
						"EAn06",
						"EAn07",
						"EAn08",
						"EAn11",
						"EAn12",
						"EAn13",
						"EAn14",
						"EAn15",
						"EAn16",
						"EAn17",
						"EAn18",
						"EDy01",
						"EDy02",
						"EDy03",
						"EDy04",
						"EDy05",
						"EDy06",
						"EDy07",
						"EDy08",
						"EDy11",
						"EDy12",
						"EDy13",
						"EDy14",
						"EDy15",
						"EDy16",
						"EDy17",
						"EDy18"
						};

//const std::vector<std::string> histoNames_v = { "EDy18"	};


double ff (double *x,double*p){return p[0]*std::exp(-(*x - p[1])*(*x - p[1])/(2*p[2]*p[2]))+p[3];};
double ff2 (double *x,double*p){return p[0]*std::exp(-(*x - p[1])*(*x - p[1])/(2*p[2]*p[2]))+p[3]   + p[4]*ROOT::Math::erfc( (*x- p[1])/( sqrt(2)*p[2])) ;};



auto myTF1 = new TF1("myGaus", ff2 , 0 ,1 , 5 );

std::vector<TH1*> h_v;
std::vector<TH1*> hFit_v;

void getSigmaCal(std::string ifilename )
{
  TFile ifile( ifilename.c_str(), "read" );
  
  TH1 * h = nullptr;
  for( auto & histoName_it : histoNames_v )
  {
    ifile.GetObject( histoName_it.c_str(), h );
    if( h )
    {
      h->GetXaxis()->SetRangeUser(550,750);
      myTF1->SetParameters(1000,662,30,200,100);
      h->Fit("myGaus","");
      double mean(h->GetFunction("myGaus")->GetParameters()[1]);
      double sigma(h->GetFunction("myGaus")->GetParameters()[2]);
      
      std::cout << h->GetName() << "\t" << mean << "\t" << sigma << "\t" << 235*sigma/mean << "%\t" <<  std::endl;
      
      h_v.push_back( (TH1*) h->Clone( std::string( std::string(h->GetName()) + "_c" ).c_str() ) );
      h_v.back()->SetDirectory(0);
      hFit_v.push_back( (TH1*)h->GetFunction("myGaus")->CreateHistogram()->Clone( std::string( std::string(h->GetName()) + "_cFit" ).c_str() ) );
      hFit_v.back()->SetDirectory(0);
    }
    
  }
  ifile.Close();
  
  TFile ofile("calFit5.root","recreate");
  for(auto & vit : h_v )
    vit->Write();
//   for(auto & vit : hFit_v )
//     vit->Write();
  
  
  ofile.Close();
  
  return;
}
Attachment 2: calFit5.root
  22   Mon May 20 09:39:23 2019 A. AlgoraDynode 08 threshold changed

Dynode 08 threshold was changed from 675 to 790. Now the rate in this detector is fine.

The global rates for the cards (dynodes and anodes) are similar.

  14   Thu May 16 06:59:51 2019 Algora Kiss NacherDet 3

Det 3 moved, both Anode and Dynode. So we have changed the HV cable to test if there are no more jumps. We used cable 9 and it was not

relabeled. The HV of the detector was corrected. It was changed to 527.5 V

  4   Wed May 15 06:40:16 2019 Algora, Kiss, Nacher DTAS aligned and calibrated

Signal cables (long cables, from preamp to digitizer) of channels 13 and 16 were changed. For the moment they have not been relabelled.

We assumed that it was not a HV supply or cable problem, since the anods were aligned and only the dynodes moved.

After changing the cables we realigned the dynodes and recalibrated all signals. Screen shots are attached.

File (root file) with the two sources (Co and Cs) saved as 201905151432_137Cs60Co.root

Configuration file: 20190515_Conf.xlsx

Rate with two sources: 52 kHz (Dynodes), 47 kHz (Anodes)

 

Attachment 1: Screenshot_from_2019-05-15_14-29-57.png
Screenshot_from_2019-05-15_14-29-57.png
Attachment 2: Screenshot_from_2019-05-15_14-30-57.png
Screenshot_from_2019-05-15_14-30-57.png
Attachment 3: Screenshot_from_2019-05-15_14-31-25.png
Screenshot_from_2019-05-15_14-31-25.png
Attachment 4: Screenshot_from_2019-05-15_14-31-55.png
Screenshot_from_2019-05-15_14-31-55.png
  25   Tue May 21 02:20:26 2019 A. AlgoraCs measurement, Cs401, 4763

Start: 10:25

Stop: 11:26

lmd: Cs137_source_201905211025_052.dl ...Cs137_source_201905211025_053.dlt

root: 201905211126_137Cs.root

Rates: 8.0 kHz (Dynodes), 8.1 kHz (Anodes)

Comment: detector  3  HV was increased by 1 V ( from 529 to 530 V). Used source CS401, 4763 as in earlier measurements.

The red box Cs source is too strong. We had 150 kHz  in the cards.

Details of the source:137Cs, 8.23x 10**3 Bq at 2010/03/16, ID: CS401, 4763

Root file attached, and tested

Attachment 1: 201905211126_137Cs.root
  102   Fri Jun 7 09:37:15 2019 The same teamCs for the AIDA synch test

Start: 17:41

Stop: 18:17

AIDA files: R19_1 (@17:57)

Dtas files: 201906071738_137Cs_AIDA_248.dlt

Comment: 137Cs (ID: XXXX) put in the centre of the DTAS on top of AIDA, with the help of the plastic ruler

  103   Fri Jun 7 12:35:14 2019 Jorge, AlvaroCorrelation time AIDA_DTAS for 60Co source
Files at mars /home/briken/190607AidaTasTest60Co
Attachment 1: AidaDTAS60CoTest.pdf
AidaDTAS60CoTest.pdf
  101   Fri Jun 7 08:47:17 2019 Jorge, Alvaro, Tom, Sunghan, AleCo 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
Screenshot_from_2019-06-07_17-09-21.png
Attachment 3: gainMatchSi.png
gainMatchSi.png
  57   Mon May 27 08:26:20 2019 A. AlgoraCo source on top of Aida

Start: 16:28

Stop: 17:03

Rates: 14.4 kHz (Dinodes), 12.8 kHz (Anodes)

Lmd:  60Co_source_AIDA_201905271627_196.dlt .... 60Co_source_AIDA_201905271627_209.dlt

Root: 201905271703_60Co_AIDA_in.root

Comments: AIDA in, sligthly less deeper than before. It is 17 mm less deeper. So from the other side we measure 17.7 mm to the nose of AIDa.

The source is on top of AIDA with a help of a plastic ruler, that it is lying on top of it. The other extreme of the ruler is attached with tape to the edge

of the frame on the beam side. The source is positioned on top of the detectors 3, and 4, in practical terms in the geometrical center, but on top of 

AIDA. 60Co source from source box (key 3). No sources around, the sources are kept inside BELEN.

Attachment 1: 201905271703_60Co_AIDA_in.root
  20   Mon May 20 07:07:59 2019 A. AlgoraCo source (CD 395)

Start: 15:10

Stop: 16:08

Positioned in the center, with the source holder.

List mode files: Co60_source_201905201510_030.dlt ... Co60_source_201905201510_034.dlt

Root file: 201905201608_60Co.root

Source: 60Co, red box, source number: CD395. 1 mm plastic (density 1.23 g/cm3)

Rates:

Dynodes: 20.5 kHz

Anodes: 12.5 kHz

 

Attachment 1: 201905201608_60Co.root
  17   Mon May 20 06:04:41 2019 A. AlgoraCo and Cs short file

Short file with the strong Co source and Cs source. To test stability
Start:11:32

Stop: 14:04

Root file: 201905201404_137Cs60Co_calib.root

Rates; 53 kHz (Dynodes), 47 kHz (anodes) So thresholds should be checked

Anode 12 (calibrated) has a large jump, because the cable in the digitizer was not fully plugged.

We need to recalibrate them. The alignment was done originally with Dynodes.

Attachment 1: Screenshot_from_2019-05-20_14-07-24.png
Screenshot_from_2019-05-20_14-07-24.png
Attachment 2: Screenshot_from_2019-05-20_14-14-15.png
Screenshot_from_2019-05-20_14-14-15.png
Attachment 3: Screenshot_from_2019-05-20_14-14-57.png
Screenshot_from_2019-05-20_14-14-57.png
Attachment 4: Screenshot_from_2019-05-20_14-15-39.png
Screenshot_from_2019-05-20_14-15-39.png
  112   Mon Jun 10 10:01:17 2019 Jose, AleCo 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
  16   Mon May 20 03:18:03 2019 A. AlgoraCo and Cs after two days

We have been running with Co and Cs for the weekend to check the overall stability.

Seems that the detectors did not move too much. Please note that the Ref detector was plugged incorrectly in channel 8

instead of channel 10 of the ancilliary card.  A new run will be done to include the reference detector.

It looks that the calibration might be sligthly shifted for detectors 12, 13,17 (Dynodes)

  27   Tue May 21 06:12:13 2019 A. AlgoraCo again, to have a root file, source CD395

Start: 14:11

Stop: 15:01

Lmd: Co60_source_201905211411_055.dlt ...Co60_source_201905211411_058.dlt

Root: 201905211501_60Co.root

Rates: 13.8 kHz (Dynodes), 12.4 kHz (anodes)

Source details: Taken from the red box. No CD395, 1 mm plastic (1.23 g/cm3)

338.4 kBq (1 July 1990). Type ASSET81 to drawing VZ-477/1E

Root file tested and attached

Attachment 1: 201905211501_60Co.root
  87   Sat Jun 1 08:25:47 2019 A. AlgoraBackground, without and with beam

Start: 16:26

Stop: 17:20 (until then no beam),

Root1: 201906011720_background_AIDA_in.root (no beam, saved 17:20), nor erased

Root2: 201906011729_background_AIDA_in.root (no beam, saved 17:29), nor erased

Root3:201906011741_background_AIDA_in.root (no beam, saved 17:41), nor erased

Root4: 201906011800_background_AIDA_in.root (with beam at the end, saved 18:00), not erased

Comment: At the begining there was no beam, to see the difference. The lead bricks blocking the way to AIDA has been removed as well as the

polyethylene blocks. The lead wall after F11 plastic remains, and of course the lead shielding and the polyethylene shielding before the DTAS is not removed.

Only the blocks that were inside the holes were removed.

Beam arrived around 17:47, intensity at F7 is 3.3 kHz, at F11 of the order of 2.4 kHz, at Aida plastic of the order of 2 kHz after substracting. The beam is centered at 102Sn, but there are a lot of other staff comming through

the noise level.

The increase in the counting rate of the NaI is very small.

Rates with NO BEAM: Dynodes 1.6 kHz, Anodes 1.9 kHz

Rates with BEAM: Dynodes 1.7 kHz, Anodes 1.9 kHz

File with guaranted no beam saved at 17:20 (201906011720_background_AIDA_in.root)

Another one saved at 17:29 (201906011729_background_AIDA_in.root), no beam also, still waiting, similarly saved at 17:41

Attachment 7 shows the rates of TF11PL (black), TCryA (blue), and TAIDAPL (the other color ?). it shows the "noise" level of the AIDA PL, and the increase in the counting

rate of the crystals.

 

Attachment 1: 201906011720_background_AIDA_in.root
Attachment 2: 20190601_Conf.xlsx
Attachment 3: 201906011729_background_AIDA_in.root
Attachment 4: 201906011800_background_AIDA_in.root
Attachment 5: Screenshot_from_2019-06-01_17-49-05.png
Screenshot_from_2019-06-01_17-49-05.png
Attachment 6: Screenshot_from_2019-06-01_18-04-02.png
Screenshot_from_2019-06-01_18-04-02.png
Attachment 7: Screenshot_from_2019-06-01_18-41-05.png
Screenshot_from_2019-06-01_18-41-05.png
  58   Mon May 27 09:12:22 2019 A. AlgoraBackground, with AIDA

Start: 17:13

Stop: 18:03

Rates: 1.8 kHz (Dynodes), 1.8 kHz Anodes

Lmd: Background_AIDA_201905271711_210.dlt ... Background_AIDA_201905271711_226.dlt

Root: 201905271803_background_AIDA_in.root

Comments: AIDA in, in the same conditions as the earlier entry. Some asymetry in the spectra is seen. See EDy05 vs EDy15 and similarly EDy03 vs EDy13

Attachment 1: Screenshot_from_2019-05-27_17-50-45.png
Screenshot_from_2019-05-27_17-50-45.png
Attachment 2: Screenshot_from_2019-05-27_17-51-02.png
Screenshot_from_2019-05-27_17-51-02.png
Attachment 3: 201905271803_background_AIDA_in.root
  50   Sat May 25 03:42:12 2019 A. AlgoraBackground, no sources around, Aida out

Start: 11:42

Stop: 14:45

Lmd: Background_201905251141_182.dlt ..Background_201905251141_186.dlt

Root: 201905251445_background.root

Comments: No sources around. All were taken back. Only doubful sources might be there, that I need to ask Nishimura san.

AIDA is out

Attachment 1: 201905251445_background.root
  61   Mon May 27 13:58:03 2019 A. AlgoraBackground, no lmd, AIDA in, no sources around

Start: 21:59

Stop: 13:15 (next day, 28/05)

Rates: 1.9-2.3 (dynodes), 1.8-1.9 kHz (anodes)

Root: 201905281315_background_AIDA_in.root

Comments: Aida inside. No sources around

Attachment 1: 201905281315_background_AIDA_in.root
  71   Wed May 29 10:01:10 2019 A. AlgoraBackground, no lmd, AIDA in

Start: 18:02

Stop: 18:33, partial file (201905291833_background_AIDA_in.root), Stop: 09:53 saved also next day (30/05) 201905300953_background_AIDA_in.root

Comments: AIDA in, Bigrips is doing settings (105Te to my best knowledge). There is a lead wall before our setting. No apparent change in the rate of background

Root: 201905300953_background_AIDA_in.root

 

Attachment 1: 201905291833_background_AIDA_in.root
Attachment 2: 201905300953_background_AIDA_in.root
  65   Tue May 28 07:49:51 2019 A. AlgoraBackground, no lmd

Start: 15:50

Stop: 10:09 (next day)

Root: 201905291009_background_AIDA_in.root

Comments: background, Aida in

  51   Sat May 25 06:53:35 2019 A. AlgoraBackground, no dlt files, last config file

Start: 14:53 (May 25)

Stop: 14: 37 (May 27)

Root: 201905271437_background.root

Comment: there is small assymetry between one side and the other. Probably it is determined by the closeness of the big wall in the direction of the beam

Attachment 1: 20190525_Conf.xlsx
  92   Mon Jun 3 01:45:31 2019 A. AlgoraBackground, no beam for a period

Start: 09:45

Stop (partial save): 09:55, 10:00, 10:14,10:29,10:37,10:46

Root: 201906030955_background_AIDA_in.root (no beam, not erased), 201906031000_background_AIDA_in.root (no beam, not erased),

201906031014_background_AIDA_in.root(no beam, not erased), 201906031029_background_AIDA_in.root(no beam, not erased),

201906031037_background_AIDA_in.root(no beam, not erased),201906031046_background_AIDA_in.root(no beam, not erased)

201906031135_background_AIDA_in.root (with beam at the end)

At 10:43 or so, a Synch pulse was sent

Intensity of the beam has been increased. There is a clear increase of the background. Rates 3.2 kHz (dynodes), 3.3 (anodes).

9 kHz at F11 plastic, 9 kHz at F7

  78   Thu May 30 08:57:34 2019 A. AlgoraBackground, no beam + beam, file not saved

Start: 16:57

Stop:

Comments: first part no beam, but later with beam

Root: File not saved

  86   Sat Jun 1 07:59:20 2019 A. AlgoraBackground, no beam

Start: approximate 15:54

Stop: 16:23

Root: 201906011624_background_AIDA_in.root

Comment: No beam. AIDA in place

 

Attachment 1: 201906011624_background_AIDA_in.root
  73   Thu May 30 02:44:56 2019 A. AlgoraBackground, just a test

Start: 11:01

Stop: 13:37

Root: 201905301337_background_AIDA_in.root

Comments: Some of the TAC spectra have desapeared with the new configuration file. To be explored.

I have tried with both configuration files that were sent.

Attachment 1: 20190530_Conf.xlsx
  82   Fri May 31 07:03:37 2019 A. AlgoraBackground, beam on, rates at F11PL and AIDAPL

Start: 15:04

Stop: partial (17:43), 201905311743_background_AIDA_in.root (file corrupt again), system will be restarted

Root:

Comment: Figure shows the rate of F11PLR (black), F11PLL (lighter color, ??) and AIDAPL (blue). There are different counting rates in left and right of F11 plastic

Attachment 1: Screenshot_from_2019-05-31_17-36-38.png
Screenshot_from_2019-05-31_17-36-38.png
  95   Mon Jun 3 12:59:31 2019 A. AlgoraBackground, beam on, 102Sn coulex

Start: 21:00

Stop: 14:24 (next day)

Root: 201906041423_background_AIDA_in.root

Comments: Beam on, rate at F7 8.9 kHz, the beam was stopped before 14:00 to change the plastic detectors at F3, F7, they are burning them

Attachment 1: 201906041423_background_AIDA_in.root
  80   Fri May 31 02:41:55 2019 A. AlgoraBackground, beam on

Start: 10:42

Stop: 11:49

Root: 201905311149_background_AIDA_in.root

Comments:

 

Attachment 1: Screenshot_from_2019-05-31_10-50-53.png
Screenshot_from_2019-05-31_10-50-53.png
Attachment 2: Screenshot_from_2019-05-31_10-50-37.png
Screenshot_from_2019-05-31_10-50-37.png
Attachment 3: Screenshot_from_2019-05-31_10-51-55.png
Screenshot_from_2019-05-31_10-51-55.png
Attachment 4: Screenshot_from_2019-05-31_10-53-05.png
Screenshot_from_2019-05-31_10-53-05.png
Attachment 5: Screenshot_from_2019-05-31_10-52-54.png
Screenshot_from_2019-05-31_10-52-54.png
Attachment 6: Screenshot_from_2019-05-31_10-55-27.png
Screenshot_from_2019-05-31_10-55-27.png
Attachment 7: 201905311149_background_AIDA_in.root
  89   Sat Jun 1 14:31:24 2019 A. AlgoraBackground, beam on

Start: 22:32

Stop: 19:18 (next day)

Comments: According to Tom, the number of ligth particles in AIDA is small

Root:201906021918_background_AIDA_in.root

Attachment 1: 201906021918_background_AIDA_in.root
  91   Sun Jun 2 12:31:45 2019 A. AlgoraBackground, beam on

Start: 20:32

Stop: 09;44

Root: 201906030944_background_AIDA_in.root

Comment: beam until 09;00

  93   Mon Jun 3 03:37:10 2019 A. AlgoraBackground, beam on

Start:11:36

Stop: 20:47

Root: 2019060312047_background_AIDA_in.root

 

102Sn beam, empty target run, Rate at F7 9 kHz

Attachment 1: 2019060312047_background_AIDA_in.root
  64   Tue May 28 06:13:27 2019 A. AlgoraBackground, Aida in

Start: 14:13

Stop: 15:47

Lmd: Background_AIDA_in_201905281413_231.dlt .. Background_AIDA_in_201905281413_233.dlt

Root: 201905281547_background_AIDA_in.root

Rates: 2.1 kHz (Dyn), 1.8 kHz (Anodes)

  90   Sun Jun 2 11:23:23 2019 A. AlgoraBackground, beam on

Start: 19:24

Stop: 20:27

Root: 201906022028_background_AIDA_in.root

Lmd:201906021924_background_AIDA_beam_on_234.dlt ..201906021924_background_AIDA_beam_on_237.dlt

Comments:  For a short period lmd file will be collected as well, to have correlations in case it is needed. Rate at F7 4 kHz

Attachment 1: 201906022028_background_AIDA_in.root
  74   Thu May 30 06:41:18 2019 A. AlgoraBackground with the beam

There was an small increase in the counting rate of the detectors after the beam was delivered. The rate at
F7 was of the order of 5 kHz. But remember that there is a lead wall protecting the detector. Root file saved. Look at TSumA for example

Root: 201905301442_background_AIDA_in.root

  76   Thu May 30 07:21:41 2019 A. AlgoraBackground with beam on

Start: 15:21

Stop: 16:41

Root: 201905301642_background_AIDA_in.root

Comments: they stopped the beam to put the target in

  75   Thu May 30 06:46:10 2019 A. AlgoraBackground with beam

Again a new test with the beam on. At the begining the beam was off and it can be noticed.

There is a lead wall after F11 plastic and in the polyethilene block there are two lead bricks to block the beam to AIDA.

201905301448_background_AIDA_in.root

201905301457_background_AIDA_in.root (beam was stopped for a short period)

Rates with the beam: 2.2 kHz (Dynodes), 2.3 (anodes)

 

 

I will not erase it and continue to collect root files (no lmd for the moment), they are still optimizing things. Rate at F11 should be similar to

the rate at F7 according to Pieter. Rate at F7 plastik  is 5 kHz. The plastik spectra (F11, our plastik) shows some spikes.

Attachment 1: 201905301448_background_AIDA_in.root
Attachment 2: 201905301457_background_AIDA_in.root
  85   Fri May 31 14:29:34 2019 A. AlgoraBackground with beam

Start: 22:29

Stop: 15:44 (next day)

Root: 201906011544_background_AIDA_in.root

Comments:

Attachment 1: 201906011544_background_AIDA_in.root
  37   Wed May 22 07:55:23 2019 A. AlgoraBackground with Aida in

Start: 15:55

Stop: 16:55

Lmd: Background_AIDA_201905221555_071.dlt

Root: 201905221655_background_with_Aida.root

Rates: 1.7 kHz (Dyn), 1.9 kHz (Anodes)

Comments: Background with AIDA in

Individual rates (kHz), remember the source is not at the center, so we expect assymetry in the counting rates):

Dy01 0.07                    An01  0.12

Dy02 0.07                  An02  0.09

Dy03 0.07                  An03  0.11

Dy04 0.08                  An04  0.07

Dy05 0.11                    An05  0.11

Dy06 0.10                    An06  0.12*

Dy07 0.08                    An07  0.10

Dy08 0.10                  An08  0.08

Dy11 0.08                   An11  0.14

Dy12 0.08                   An12  0.09

Dy13 0.08                   An13  0.12

Dy14 0.10                   An14  0.10

Dy15  0.09                  An15  0.16

Dy16 0.10                   An16  0.10

Dy17 0.09                   An17  0.14

Dy18 0.11                   An18  0.10

Attachment 1: 201905221655_background_with_Aida.root
  39   Wed May 22 09:44:57 2019 A. AlgoraBackground with AIDA in

Start: 17:46

Stop: 10:14 (next day)

Lmd: Background_AIDA_201905221746_075.dlt ..Background_AIDA_201905221746_081.dlt

Root: 201905231014_background_with_Aida.root

Rates: 1.6 kHz (Dyn), 1.8 kHz (Anodes)

Comments: Background with AIDA in

Individual rates at the end of the measurement (kHz), remember the source is not at the center, so we expect assymetry in the counting rates):

Dy01 0.08                   An01  0.12

Dy02 0.07                  An02  0.09

Dy03 0.08                  An03  0.11

Dy04 0.08                  An04  0.07

Dy05 0.12                   An05  0.11

Dy06 0.11                   An06  0.11

Dy07 0.08                    An07  0.10

Dy08 0.11                  An08  0.08

Dy11 0.09                   An11  0.14*

Dy12 0.08                   An12  0.09

Dy13 0.08                   An13  0.12

Dy14 0.10                   An14  0.11

Dy15  0.11                  An15  0.15

Dy16 0.12                   An16  0.11

Dy17 0.09                   An17  0.14

Dy18 0.09                   An18  0.10

Attachment 1: 201905231014_background_with_Aida.root
  77   Thu May 30 08:43:29 2019 A. AlgoraBackground no beam

Start: 16:43

Stop: 16:56

Root: 201905301656_background_AIDA_in.root

Comment: no beam, AIDA in

Rates: 1.5 kHz (Dynodes), 1.8 kHz (Anodes)

  48   Fri May 24 12:32:48 2019 A. AlgoraBackground measurement, no sources around

Start: 20:32

Stop: 10:05

Lmd: Background_201905242032_111.dlt ...Background_201905242032_114.dlt

removed the rest of the files. Ocupying too much space

Root: Background_201905242032_111.dlt (temporary) to play (until 21;11),

full: 2019052521005_background.root

Comment: all sources were taken back. Check for assymetry.

Attachment 1: 201905242111_background.root
Attachment 2: 2019052521005_background.root
  108   Mon Jun 10 04:14:39 2019 Ale, JoseBackground measurement overnight
Start:~14:00 (June 9)
Stop:10:30

File: 201906101030_background_AIDA_in.root
  43   Fri May 24 06:25:14 2019 A. AlgoraBackground assymetry

Some pictures after the background during the nigth. The front and back side looks asymetric. To be checked again with a 137Cs source.

AIDA is in. Root file is saved, after one night.

Root: 201905241444_background_with_Aida.root

 

 

Attachment 1: Screenshot_from_2019-05-24_14-40-25.png
Screenshot_from_2019-05-24_14-40-25.png
Attachment 2: Screenshot_from_2019-05-24_14-38-02.png
Screenshot_from_2019-05-24_14-38-02.png
Attachment 3: 201905241444_background_with_Aida.root
  10   Wed May 15 11:53:17 2019 Algora, Nacher, KissBackground

Start: 20:05

Stop: 09:44

Background rate 2.9 kHz (Dynodes), 2.3 (Anodes)  (Threshold of detector 13 was increased)

Files: Background_20190515_006.dlt ...  _014.dlt

Root file: 201905160944_bckg_overnight.root (attached)

 

Pulser self-triggered at 100Hz

Attachment 1: 201905160944_bckg_overnight.root
  26   Tue May 21 03:35:10 2019 A. AlgoraBackground

Start: 11:34

Stop: 13:52

Rates: 1.7 kHz (Dynodes) 2.0 kHz (Anodes)

Root: 201905211352_background.root

Lmd: Background_201905211134_054.dlt

After a fantastic shower, since it is raining cats and dogs ....

Attachment 1: 201905211352_background.root
  30   Tue May 21 07:50:03 2019 A. AlgoraBackground

Start: 15:49

Stop: 16:49

Lmd: Background_201905211549_063.dlt

Root: 201905211649_background.root

Rates: 1.7 kHz (dynodes) 1.9 kHz (anodes)

Comment: All measurements have been done with the pulser set to 10 Hz. We should think if this have to be increased

Attachment 1: 201905211649_background.root
  32   Tue May 21 09:52:43 2019 A. AlgoraBackground

Start: 17:53

Stop: 18:53

Rates: 1.8 kHz (dynodes),  1.9 kHz (anodes)

Lmd: Background_201905211753_067.dlt

Root:  201905211853_background.root

Comments: We will continue measuring, but only for a while with Listmode

  33   Tue May 21 10:54:24 2019 A. AlgoraBackground

Start: 18:55

Stop: 20:01

Lmd: Background_201905211855_068.dlt

Root:201905212001_background.root

Rates: 1.7 kHz (Dyn), 1.9 kHz (Anodes)

Comment: all measurements of today can be used to characterize the full detector.

Sources were possitioned in the center of the spectrometer, with the piece created at Ific

  83   Fri May 31 09:49:08 2019 A. AlgoraBackgroun, beam on

Start: 17:49

Stop: 22:11

Root: 201905312211_background_AIDA_in.root

Comments:

  52   Sat May 25 07:04:52 2019 A. AlgoraAncilliary card used channels until now

For the moment there are three channels connected.

Channel 5 is AIDA plastic,

Channel 10 is the anode of the Ref detector

Channel 16 is the pulser.

  144   Wed Jun 19 05:10:15 2019 AlvaroAida plastic - gain change
TAC AIDAPL - CryA changed
After increasing the gain, x2 peaks in TAC
Attachment 1: changeGainAPL.png
changeGainAPL.png
  69   Wed May 29 09:08:11 2019 A. AlgoraAIDA plastic setting changed

AIDA plastic changed.

HV was at 1000 V, it was changed to 1300 V

Coarse gain was changed to x5, Fg remains as it was.

I had only two minutes to enter (it was a rush). Better to verify it again

  104   Sat Jun 8 04:22:39 2019 Jorge AlvaroAIDA TAS correlation with 137Cs
Files at mars /home/briken/190607AidaTasTest137Cs
For this experiment TAS Signal is stored 
Attachment 1: BetaTas137Cs.png
BetaTas137Cs.png
Attachment 2: BetaGAmma137Cs.png
BetaGAmma137Cs.png
  119   Fri Jun 14 16:22:25 2019 AT, OH, JA, CG, TDAIDA Sync
Problem with the sync checker appeared AIDA was not its notmal 14us out from DTAS.

Check with source shows we are in sync still

AIDA files R34_1 and R34_2
Attachment 1: AIDACorrelation.png
AIDACorrelation.png
  55   Mon May 27 07:18:26 2019 A. AlgoraAIDA Plastik

Nishimura san found the module used for the AIDA plastik in the last BRIKEN run. We put it instead of the TFA. It was kept in the same

setting conditions as in the earlier experiment.

AIDA plastic module configuration (Ortec 671 Amplifier)

Coarse gain: 20

Fine gain: ?

Shaping time (us): 0.5

Type: Gaus

Signal pos

The configuration of the digitizer might need  to be updated (5)

  47   Fri May 24 10:57:37 2019 A. Algora60Co, AIDA out, possitioned 5 mm deeper

Start: 18:58

Stop: 20:20

Lmd:  60Co_source_201905241858_095.dlt ...60Co_source_201905241858_106.dlt

Root: 201905242020_60Co.root

Comments: AIDA out. The source is possitioned 5 mm deeper as in the earlier Cs measurement (same position as the earlier entry)

To check asymmetry effects

Attachment 1: 201905242020_60Co.root
  49   Sat May 25 02:11:09 2019 A. Algora60Co source, red box, no sources around, No AIDA

Start: 10:27

Stop: 11:31

Root: 201905251131_60co.root

Lmd: 60Co_source_201905251027_176.dlt ...60Co_source_201905251027_181.dlt

Comments: possitioned as the measurements of yesterday. 5 mm deeper than earlier.

Red box with the other sources inside BELEN, far away from the DTAS

A few detectors have moved, but for the moment I will not correct it.

Reference detector in channel 10. It is very noisy now. I changed the threshold from 1400 to 1600 but still noisy. It requires further attention

New Config file saved.

Attachment 1: 201905251131_60co.root
Attachment 2: 20190525_Conf.xlsx
  23   Mon May 20 10:02:43 2019 A. Algora60Co again, with better threshold settings

Start: 18:06

Stop: 20:20

Rates: 14 kHz (Dynodes) 12.7 kHz (anodes)

Lmd: Co60_source_201905201806_037.dlt ...Co60_source_201905201806_045.dlt

Root:  201905202020_60Co.root

Attachment 1: 201905202020_60Co.root
  38   Wed May 22 09:01:43 2019 A. Algora60Co (source CD 395) with AIDA in

Start: 17:00

Stop: 17:40

Lmd:  Co60_source_AIDA_201905221700_072.dlt ..Co60_source_AIDA_201905221700_074.dlt

Root: 201905221740_60co_with_Aida.root

Rates: 13.2 kHz (Dyn), 12.6 kHz (Anodes)

Comments: 60Co source with AIDA in, red box, CD 395 . The source is not centered. It is positioned (the center of the source) at 14.6 cm

from the beam side external edge of the frame (lower NaI numbers). The holder is touching the nose of AIDA.

The nose of AIDA is 16 cm from the external edge of the frame (down stream). In that position Si # 3 is at the center of the DTAS according to Tom.

We have to be very careful when AIDA is moved in. Some of the AIDA  flat connector cables are touching the connectors of our NaI cables.

Individual rates (kHz), remember the source is not at the center, so we expect assymetry in the counting rates):

Dy01 2.2                    An01  2.27

Dy02 0.88                  An02  0.91

Dy03 2.08                  An03  2.20

Dy04 0.87                  An04  0.86

Dy05 2.10                    An05  2.17

Dy06 0.90                    An06  0.89

Dy07 2.01                    An07  2.13

Dy08 0.93                  An08  0.93

Dy11 0.60                   An11  0.68

Dy12 0.36                   An12  0.33

Dy13 0.57                   An13  0.62

Dy14 0.35                   An14  0.33

Dy15  0.58                  An15  0.65

Dy16 0.35                   An16  0.33

Dy17 0.54                   An17  0.62

Dy18 0.32                  An18  0.31

Attachment 1: 201905221740_60co_with_Aida.root
  29   Tue May 21 07:07:36 2019 A. Algora22Na, source 700

Start: 15:08

Stop: 15:42

Rates: 19 kHz (Dynodes), 16 kHz (anodes)

Lmd: Na22_source_201905211508_059.dlt ...Na22_source_201905211508_062.dlt

Root: 201905211543_22Na.root

Source details: 22Na, ID NA 401, 700, 1.038 x 105 Bq (2010/03/16), key 5,

It appears in the Sunflower home page as 09-7007 with an estimated activity of 8.9 Bq/s today

Comment; seems dynode 4 moved a little up. Most detectors keep a reasonable alignment

When overlay was marked, it did not save the root file. Root attached and tested

Attachment 1: 201905211543_22Na.root
  31   Tue May 21 08:55:20 2019 A. Algora152Eu, source ID 272

Start: 16:56

Stop: 17:46

Rates: 12.6 kHz (dynodes), 12 kHz (anodes)

Lmd: Eu152_201905211656_064.dlt ... Eu152_201905211656_066.dlt

Root: 201905211746_152Eu.root

Source details: 152Eu, ID: EU401, 272, 1.06x10**4 Bq (2010/03/16), key 9

Comments:

Attachment 1: 201905211746_152Eu.root
  46   Fri May 24 09:43:49 2019 A. Algora137Cs source, AIDA out, to check assymetry

Start: 17:43

Stop: 18:51

Root: 201905241851_137Cs.root

Lmd:  137Cs_source_201905241744_087.dlt...137Cs_source_201905241744_094.dlt

Comments: AIDA out. The source is positioned 5 mm deeper than before from the holder side (the arm is 5 mm longer).

To check if the assymetry is reduced.

Attachment 1: 201905241851_137Cs.root
  40   Thu May 23 02:48:29 2019 A. Algora137Cs short run with AIDA in

Start: 10:48

Stop: 10:58

Root: 201905231058_137Cs_with_Aida.root

Comment: Aida in, source in the position as in the earlier entries. Just to check if there is any jump. No lmd, only root.

No large displacements. Det Dyn1 seems to have slightly larger statistics. The assymetry of the two sides is clear, as it should be.

 

Attachment 1: 201905231058_137Cs_with_Aida.root
  54   Mon May 27 07:15:06 2019 A. Algora137Cs run, AIDA out, source in the center

Start: 15:15

Stop: 15:31

Lmd: 137Cs_source_201905271514_187.dlt .. 137Cs_source_201905271514_195.dlt

Root: 201905271531_137Cs.root

Rates: 7.9 kHz (Dynodes), 7.9 kHz (Anodes)

Comments: Aida out, source in the center. As in earlier measurements 5 mm deeper.

Reference detector might require repositioning of the optical fiber. It appears too close to the Cs peak and it is very noisy.

 

 

Attachment 1: 201905271531_137Cs.root
  35   Wed May 22 06:31:54 2019 A. Algora137Cs quick test of alignment

Start: 14:32

Stop: 14:37

Source: 137Cs

Comments: Detectors show small drifts, of the order of the precision of the HV (we could apply 0.5 V corrections to align some of them, but I will not touch them now)

Dy16 looks quite off in the background measurement, but not with the Cs one !!!.

Calibrated spectra: Dy3 an An3 moved a little in the same direction, An12 looks also a little displaced.

Now I plan to measure some sources with AIDA in. It means that the sources will not be centered. The available distance from the oposite side to

the nose of AIDA is 16 cm.

Attachment 1: 201905221437_137Cs.root
  9   Wed May 15 11:50:04 2019 Algora, Nacher137Cs listmode, and rootfile

137Cs source in the center of the DTAS, with the IFIC holder

list mode files: Cs137_Source_20190515_000.dlt to Cs137_Source_20190515_005.dlt

Root file: 201905151942_137Cs.root

 

Attachment 1: 201905151942_137Cs.root
  36   Wed May 22 07:15:00 2019 A. Algora137Cs (4763) with AIDA in

Start: 15:15

Stop: 15:50

Lmd:  Cs137_source_AIDA_201905221515_069.dlt ..Cs137_source_AIDA_201905221515_070.dlt

Root: 201905221550_137Cs_with_Aida.root

Rates: 7.5 kHz (Dyn), 7.8 kHz (Anodes)

Comments: 137Cs source with AIDA in, Source CS401, 4763. The source is not centered. It is positioned (the center of the source) at 14.6 cm

from the beam side external edge of the frame (lower NaI numbers). The holder is touching the nose of AIDA.

The nose of AIDA is 16 cm from the external edge of the frame (down stream). In that position Si # 3 is at the center of the DTAS according to Tom.

We have to be very careful when AIDA is moved in. Some of the AIDA  flat connector cables are touching the connectors of our NaI cables.

Individual rates (kHz), remember the source is not at the center, so we expect assymetry in the counting rates):

Dy01 1.1                    An01  1.2

Dy02 0.35                  An02  0.36

Dy03 0.97                  An03  1.0

Dy04 0.34                  An04  0.36

Dy05 1.1                    An05  1.1

Dy06 0.4                    An06  0.41

Dy07 1.0                    An07  1.1

Dy08 0.37                  An08  0.37

Dy11 0.27                   An11  0.33

Dy12 0.15                   An12  0.16 

Dy13 0.25                   An13  0.28

Dy14 0.15                   An14  0.16

Dy15  0.28                  An15  0.33

Dy16 0.15                   An16  0.15

Dy17 0.25                   An17  0.31

Dy18 0.16                   An18  0.15

 

Attachment 1: 201905221550_137Cs_with_Aida.root
  63   Tue May 28 05:43:41 2019 A. Algora133Ba source. (IR052 from the third floor)

Start: 13:43

Stop: 14:05

Comments: The source looks also too strong. Rates: 39 kHz (Dynodes), 40 kHz (anodes).

Source ID: IR052 from the third floor, small plastic rectangular form

Rates:

RefAn: 180 Hz

Dy01: 3.7 kHz

Dy02: 0.4 kHz

Dy11: 0.5 kHz

Dy12: 0.13 KHz

AIDA in. The source is put at the extreme of the source holder, at 16.5 cm from the edge of the detectors. Almost touching AIDA.

Lmd: 133Ba_source_AIDA_in_201905281343_227.dlt ..133Ba_source_AIDA_in_201905281343_230.dlt

Root: 201905281405_133Ba_AIDA_in.root

  41   Thu May 23 03:06:15 2019 A. Algora133Ba source of red box too strong

The Ba source of the red box is too strong. We can not use it. I need to identify the other one, which does not appear to be in RIBF.

The counting rate was 74 kHz in the DTAS.

ELOG V3.1.4-unknown