 Sat Jun 15 20:43:50 2019, Pancho & Kike, root file data 2:30 - 4:30 
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| corresponding to runs .dlt 12-14 |
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Sat Jun 15 18:39:07 2019, Pancho & Kike, root files
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| 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 |
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Sat Jun 15 18:38:15 2019, Pancho & Kike, run 12
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Shifters: Pancho & Kike
Degrader: none
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Sat Jun 15 18:15:08 2019, Pancho& Kike, run 9 9x
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Shifters: Pancho & Kike
Degrader: none
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Fri Jun 14 16:22:25 2019, AT, OH, JA, CG, TD, AIDA Sync
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Problem with the sync checker appeared AIDA was not its notmal 14us out from DTAS.
Check with source shows we are in sync still
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Wed Jun 12 02:04:07 2019, AA, EN, PM, AT, background during in-beam exp.
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In-beam experiment going on. Only 12h of beam in the last 21h.
Start: ~1pm (11th-June)
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Tue Jun 11 01:45:55 2019, Pancho, Ale, background
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Start: 09:46
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Mon Jun 10 13:02:16 2019, Jose, Pancho, Ale, background, Aida in 8x
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Start: 21:03
Stop: 09:30
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Mon Jun 10 12:48:01 2019, Ale, Jose, New Config file 6x
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Conf file with new calibration:
20190610_2035_Conf_DTAS.xlsx
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Mon Jun 10 12:31:52 2019, Ale, Jose, New calibration
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New calibration with more statistics
File: 20190610_2030_60Co_137Cs_AIDA_in.root
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Mon Jun 10 10:44:36 2019, Ale, Jose, New Conf file with new calibration
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| File: 20190610_1835_Conf_DTAS.xlsx |
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Mon Jun 10 10:01:17 2019, Jose, Ale, Co and Cs for new calibration
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Start: 17:57 ?
Stop:18:15
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Mon Jun 10 09:58:42 2019, Jose, Ale, Gain matching
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| We have corrected small gain changes by changing the HV of detectors. Attached are the new values |
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Mon Jun 10 08:07:17 2019, Ale, Jose, Test of pulser count rates
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File: 20190610_1602_background_AIDA_in.root
SyncPulse: 61777
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Mon Jun 10 04:18:24 2019, Ale, Jose, New Configuration File
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File: 20190610_1145_Conf_DTAS.xlsx
Several changes and corrections
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Mon Jun 10 04:14:39 2019, Ale, Jose, Background measurement overnight
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Start:~14:00 (June 9)
Stop:10:30
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Sun Jun 9 04:03:38 2019, Jorge, Jose, Pancho, Alvaro, Kike, Ale, effect of the pulser in the low energy part of the anodes
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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 |
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Sun Jun 9 03:59:40 2019, Many, some cable changes
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| The cable of detector 8 was changed (long cable) to reduce the noise. The cable (long) of the reference detector was also changed. |
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Sat Jun 8 04:38:30 2019, Nacher, Algora, Tain, Molina, source top and bottom
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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: |
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Sat Jun 8 04:22:39 2019, Jorge Alvaro, AIDA TAS correlation with 137Cs
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Files at mars /home/briken/190607AidaTasTest137Cs
For this experiment TAS Signal is stored |