AIDA GELINA BRIKEN nToF CRIB ISOLDE CIRCE nTOFCapture DESPEC DTAS EDI_PSA 179Ta CARME StellarModelling DCF K40
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Entry  Wed May 22 06:31:54 2019, A. Algora, 137Cs quick test of alignment 201905221437_137Cs.root

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.

Entry  Wed May 22 07:15:00 2019, A. Algora, 137Cs (4763) with AIDA in 201905221550_137Cs_with_Aida.root

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

 

Entry  Wed May 22 07:55:23 2019, A. Algora, Background with Aida in 201905221655_background_with_Aida.root

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

Entry  Wed May 22 09:01:43 2019, A. Algora, 60Co (source CD 395) with AIDA in 201905221740_60co_with_Aida.root

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

Entry  Wed May 22 09:44:57 2019, A. Algora, Background with AIDA in 201905231014_background_with_Aida.root

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

Entry  Thu May 23 02:48:29 2019, A. Algora, 137Cs short run with AIDA in 201905231058_137Cs_with_Aida.root

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.

 

Entry  Thu May 23 03:06:15 2019, A. Algora, 133Ba 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.

Entry  Thu May 23 04:18:57 2019, A. Algora, SY2527 fixed  

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

Entry  Fri May 24 06:25:14 2019, A. Algora, Background assymetry Screenshot_from_2019-05-24_14-40-25.pngScreenshot_from_2019-05-24_14-38-02.png201905241444_background_with_Aida.root

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

 

 

Entry  Fri May 24 07:57:51 2019, A. Algora, Lead 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.

Entry  Fri May 24 08:33:52 2019, A. Algora, background, AIDA is out 201905241730_background.root

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

Entry  Fri May 24 09:43:49 2019, A. Algora, 137Cs source, AIDA out, to check assymetry 201905241851_137Cs.root

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.

Entry  Fri May 24 10:57:37 2019, A. Algora, 60Co, AIDA out, possitioned 5 mm deeper 201905242020_60Co.root

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

Entry  Fri May 24 12:32:48 2019, A. Algora, Background measurement, no sources around 201905242111_background.root2019052521005_background.root

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.

Entry  Sat May 25 02:11:09 2019, A. Algora, 60Co source, red box, no sources around, No AIDA 201905251131_60co.root20190525_Conf.xlsx

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.

Entry  Sat May 25 03:42:12 2019, A. Algora, Background, no sources around, Aida out 201905251445_background.root

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

Entry  Sat May 25 06:53:35 2019, A. Algora, Background, no dlt files, last config file 20190525_Conf.xlsx

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

Entry  Sat May 25 07:04:52 2019, A. Algora, Ancilliary 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.

Entry  Mon May 27 07:11:22 2019, A. Algora, detectors realigned with Cs Screenshot_from_2019-05-27_15-13-09.png

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

All detectors were realigned

Entry  Mon May 27 07:15:06 2019, A. Algora, 137Cs run, AIDA out, source in the center 201905271531_137Cs.root

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.

 

 

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