| ID |
Date |
Author |
Category |
Subject |
Text |
 |
|
81
|
Sat May 8 21:10:24 2021 |
Michael, Ruijiu, Helmut, Yuri, Wolfram, Sergey, Shahab | Runs | started data taking with high resolution | after optimizing the scrapers we have reached
the highest possible resolution in the isochronous
mode.
|
|
|
82
|
Sat May 8 21:42:26 2021 |
All | Runs | Stop72Ge | |
|
|
84
|
Sat May 8 22:06:36 2021 |
Michael, Ruijiu, Helmut, Yuri, Wolfram, Sergey, Shahab | Runs | stopped data taking with the high resolution | last file names with this setting:
245: 2021.05.08.20.42.03.743.tiq
|
|
|
87
|
Sun May 9 02:19:04 2021 |
Jacobus, Shahab | Runs | First 52Mn run | Run E143-245 MHz-2021.05.09.01.17.42.265.tiq
is the first run of the experiment on 52Mn. |
|
|
88
|
Sun May 9 02:32:58 2021 |
Jacobus, Shahab | Runs | possible 52-Mn isomer | the intensity of the line on the left side
is so high, it is difficult to see the isomers
in the middle as can be seen in the auto |
|
|
89
|
Sun May 9 02:45:50 2021 |
Jacobus, Michele, Shahab | Runs | Example of possible 52.Mn isomer | this is how it should look like |
|
|
90
|
Sun May 9 02:51:44 2021 |
Iris | Runs | Example of possible 52.Mn isomer | So the "isomers" pop up at ~-600 Hz and +580
Hz... is the -600 Hz on the left the 378
keV isomer (21 min) and the +580 Hz on the |
|
|
91
|
Sun May 9 03:24:12 2021 |
Iris (Shahab, Jacobus, Chris G., Michele) | Runs | Example of possible 52.Mn isomer | Short update from Yuri: these are not our
isomers. These are 45Sc (left, 12 keV isomer
not resolvable) and 75Br (center), and the |
|
|
92
|
Sun May 9 04:15:50 2021 |
Michele, Jacobus, Shahab | Runs | Beam issues for short duration |
ESR warning (colour red in the panel)
|
|
|
93
|
Sun May 9 05:11:55 2021 |
Iris (Chris G., Jacobus, Michele) | Runs | First 52Mn run (no 52Mn unfortunately) | > Run E143-245 MHz-2021.05.09.01.17.42.265.tiq
is the first run of the experiment on 52Mn.
|
|
|
98
|
Sun May 9 06:15:09 2021 |
Iris, Chris G., Jacobus, Michele | Runs | Triplet: zoom in | Zoom into the triplet: the satellite peaks
on the right are clearly visible.
This is just one file but one *might* see |
|
|
104
|
Sun May 9 13:15:38 2021 |
Liliana Andrew | Runs | Stopped data taking during modifications for the beam energy | Beam energy to be increase to move Mn into
the ring.
First step we set the energy to 445 MeV. |
|
|
107
|
Sun May 9 16:19:06 2021 |
Rodostina, Oliver, Wolfram, Shahab | Runs | Setting to 52Mn ???? | first filename in this recording:
E143-245MHz-2021.05.09.15.16.49.816.tiq |
|
|
109
|
Sun May 9 18:41:33 2021 |
Rodostina, Oliver, Wolfram, Helmut, Yuri, Shahab | Runs | stopped data taking for energy change | last recorded filename:
E143-245MHz-2021.05.09.17.38.44.410.tiq
|
|
|
111
|
Sun May 9 19:03:02 2021 |
Rodostina, Oliver, Wolfram, Helmut, Yuri, Shahab | Runs | quadrupoles were down, fixed. | |
|
|
113
|
Sun May 9 20:39:17 2021 |
Shahab | Runs | Subtracting the background | still in the search of 70-Se |
|
|
117
|
Sun May 9 23:28:25 2021 |
Kanika, Alex, Wolfram, Helmut, Shahab | Runs | return with the Ge setting of the last night | starting filenames:
E143-410MHz-2021.05.09.23.28.24.018.tiq
|
|
|
129
|
Mon May 10 06:16:31 2021 |
Kanika, Alex, Shahab | Runs | Recording broad band spectra with 410 | doing some broadband spectra recording with
the 410 MHz detector, for the purpose of
future confirmation of identification lines. |
|
|
131
|
Mon May 10 06:35:58 2021 |
Kanika, Alex, Shahab | Runs | going back to shot by shot recording with 410 detector | going back to shot by shot recording with
410 detector |
|
|
140
|
Tue Jun 29 21:10:30 2021 |
Shahab | Runs | 72-Ge setting | the new setting is roughly 400 khz lower in
frequency.
Previous beam time Ge was on 243.100 now |
|