| Status |
ExpNbr |
Date |
Author |
Type |
Category |
Target-Source |
Subject |
Text |
 |
| Fixed | com2019 |
Sat Apr 6 06:24:04 2019 |
mugast | RUN | Software | CD2 | new data 5more statistics° | |
|
| Fixed | e768s |
Wed Jul 17 01:08:03 2019 |
mugast | VAMOS | General | LiF | new beam settings | The last values Q32=21.0, Q31=22.8
With these new optimzed values, we have:
|
|
| Fixed | e744s |
Sat Apr 13 17:31:54 2019 |
mugast | VAMOS | Hardware | | new Threshold on DC1 Channel 127 | Channel 127 of DC1 had a reduction of gain
from yesterday, I corrected the gain by calibration
and I reduced the threshold from 2114 to |
|
| Fixed | e744s |
Mon Apr 15 15:36:48 2019 |
iulian Francois Fairouz Catalin | OFFLINE | General | CH2 | looking for gamma proton events | elab_Brho_gamma_thetaCond_int_ThinTar.pdf
-> thin target ELab protons vs Brho 14O
in M/Q for protons mult 1 in MUGAST. Orange |
|
| Fixed | e744s |
Fri Apr 12 13:53:56 2019 |
diego | OTHER | General | | intervention | TAC FPMW_HF in VAMOS was still out of range
for MUGAST physics
We increased the range from 1us to 2us and |
|
| Fixed | TEST |
Mon Feb 24 10:26:29 2020 |
Marlène | GRIT | General | | infos | We have changed the range of the TAC FAG-HF
to 500ns (it was 200 ns before)
|
|
| Fixed | e768s |
Fri Jul 19 13:24:01 2019 |
mugast | OFFLINE | General | LiF | g-ray spectrum (run 112) requiring 19Ne in VAMOS | |
|
| Fixed | e744s |
Sat Apr 13 17:03:14 2019 |
Jérémie & François | OFFLINE | General | | first gamma spectrum | After a few hours run. |
|
| Fixed | e744s |
Sun Apr 14 03:30:28 2019 |
Iulian Iulia | OFFLINE | Social | CH2 | first calculation ECM ThetaCM for gamma-P emission | |
|
| Fixed | e768s |
Sat Jul 27 11:02:13 2019 |
mugast | ONLINE | General | | figures run 152 | |
18x |
| Fixed | e744s |
Tue Apr 16 00:04:08 2019 |
beyhan | OFFLINE | General | | ewire evolution vs beam intensity (normalized to CATS intensity) | |
|
| Fixed | |
Mon Apr 8 07:54:53 2019 |
iulian | MUST2 | Hardware | | end alpha contamination run | Problem M3 EY , moving piedestal... See below
Alfa spectra have changed, no longer continuous
excepting partially MM2. |
|
| Fixed | e793s |
Fri Mar 12 03:57:46 2021 |
Taras, Nishu, Chloe, Charlie | VAMOS | General | CD2 | dipole issue fixed | the alimentation on dipole (G1.G.D4.P) was
turned off,
the value was resetted(322.6) and works fine |
|
| Fixed | e744s |
Tue Apr 16 01:01:42 2019 |
beyhan, louis, serge, | OFFLINE | General | | different parameters evolution as function of intensity | |
6x |
| Fixed | e768s |
Sat Jul 27 21:12:47 2019 |
teodora & beyhan | OTHER | Hardware | | cout rate with no beam & water level check | Around 9 pm, we observed an average count
rate of 30kHz on the "or agata" scaler rates
panel of GECO. The other count rates were |
6x |
| Fixed | e793s |
Tue Mar 16 04:06:46 2021 |
Lynda, Cyril, Nishu | AGATA | General | CD2 | counting rates AGATA | crystal 12B counting rate is too low ~ 5 /
s compared to an average of ~ 80/s - 100/
s for the other crystals
|
|
| Fixed | com2019 |
Sat Apr 6 13:10:11 2019 |
mugast | VAMOS | Hardware | CD2 | check in VAMOS HV | target drift chamber HV checked. They are
OK |
|
| Fixed | e744s |
Thu Apr 11 17:37:29 2019 |
Valérian, Chloé and François | OTHER | Hardware | | changes in the electronic | Changes made in the electronic during the
break between 14N and 14O
|
|
| Fixed | e744s |
Thu Apr 11 18:08:12 2019 |
Marlène | OTHER | Hardware | | changes in the electronic | [quote="Valérian, Chloé and François"]Changes
made in the electronic during the break between
14N and 14O
|
|
| Fixed | e744s |
Mon Apr 15 09:59:32 2019 |
Marlène | RUN | General | CH2 | change thresholds in DSSD MUST2 and suppression CsI | From RUN126
change of MUST2 DSSD thresholds : thresholds
are 583 keV now
|
|