| Status |
ExpNbr |
Date |
Author |
Type |
Category |
Target-Source |
Subject |
| Fixed | com2019 |
Sat Apr 6 08:18:55 2019 |
mugast | RUN | Software | CD2 | Online Scalers run 256 @8h00 am 06/04 for reference |
|
| Fixed | com2019 |
Sat Apr 6 10:57:35 2019 |
Nicolas | OFFLINE | Software | CD2 | time of flight v.s. energy in MUGAST (run 256, all stat) |
|
| Fixed | com2019 |
Sat Apr 6 11:40:08 2019 |
mugast | OFFLINE | Software | CD2 | AGATA spectrum in coincidence with MUGAST VAMOS run 256 |
|
| Fixed | com2019 |
Sun Apr 7 14:24:18 2019 |
Valerian | OFFLINE | Software | CD2 | Ex and E gamma with all statistic (run 256+257) |
|
| Fixed | com2019 |
Tue Apr 9 10:44:40 2019 |
Valerian | MUST2 | Software | CD2 | CsI Calib files from the commissioning for proton |
| CsI calibration obtained from the proton data of the commissioning of mugast. |
| Fixed | e744s |
Tue Apr 9 18:08:22 2019 |
Marlène and François | DAQ | Software | | new inputs in the ADC Mugast |
new inputs in the ADC mugast
T_Mugast_HF = input N°2
E_AGATA = agata 42 = input N°3
T_AGATA_HF = N° 4
gains of the signal AGATA 42 were changed from 200 to 50
|
| Pinned | e744s |
Wed Apr 10 11:57:37 2019 |
A. Lemasson | OFFLINE | Software | | VAMOS Conversion HowTo |
HOW TO convert a run in VAMOS
- Do : source $HOME/GoToVamosAna
- To Convert a Run : MyVAna -d2Ar <RunNr>
- Otherwise, If you want to convert a single file : MyVAna -d2Ar -f <Infile> <OutFile>
- Output Root rile is written to : ./RootA/
If you encounter the error on Brho "Could not find the BrhoRef for the run <RunNr> ", Update the ./Calibs/ListBrho.dat file with relevant Brho for RunNr |
| Pinned | e786s |
Wed Apr 10 13:30:48 2019 |
Valerian, Adrien and Antoine (edit by Louis) | OFFLINE | Software | N/A | How to perform analysis for e786s |
Here is the updated procedure to convert a run, with VAMOS data and add those data to the Kinematic plot.
Every 4Go there will be a file change, to see if there is a file change do :
- ls -ltrh /data/mugastX/e786s/acquisition/run/
convert the last 4Go file and add it to the chain using the following step:
Step O: Take your favorite ortholinear keyboard (optional)
Step 1: Login the VAMOS environment and convert the run :
Open a terminal from one of the mugast computer:
- Type: source $HOME/GoToVamosAna
- Type: MyVAna -d2Ar -f /data/mugastX/e786s/acquisition/run/run_$$$$-DD-MM-YY.HHhMMmSSs /data/mugastX/e786s/acquisition/RootA/r$$$$_000a.root
OR
- Type: MyVAna -d2Ar -f /data/mugastX/e786s/acquisition/run/run_$$$$-DD-MM-YY.HHhMMmSSs.N /data/mugastX/e786s/acquisition/RootA/r$$$$_00Na.root
(If you encounter the error on Brho "Could not find the BrhoRef for the run <RunNr> ", Update the ./Calibs/ListBrho.dat file with relevant Brho for RunNr)
Step 2: Analyse the file using the npanalysis program:
- Type: exit (<-this exit the environment of VAMOS)
- Type: lpcgrit (<-this load the analysis environment )
- Type: npp MUGAST
- Type: edit the exe.sh to treat releverant run. command should be: npanalysis -D mugast.detector -C Calibration.txt -E ./Reaction/46Ar3Hed.reaction -T ./offline/root_e786svamos/r$$$$_00Na.root AD -O run_$$$$_N.root
(This could be used with any file, either from Offline conversion, or the VAMOS Analysis conversion or the Merged Tree from AGATA)
The run will be created in the NPOutputs folder |
| Fixed | e744s |
Thu Apr 11 11:36:09 2019 |
Valerian | OFFLINE | Software | CH2 | Comparison between the two e744 |
| Current calibration is off, a shift of -1.5MeV was done to reproduce the previous data. |
| Fixed | e744s |
Thu Apr 11 13:43:26 2019 |
Valerian | OFFLINE | Software | CH2 | Target position for 14N runs |
|
| Fixed | e744s |
Thu Apr 11 16:07:59 2019 |
Valerian and Louis | OFFLINE | Software | CH2 | HF resolution |
| Using the value of the HF=83,4ns. We can obtain the calibrated plot of T_CATS2_HF which is joined and gives us roughly a 2-3 ns resolution for the HF |
| Fixed | e744s |
Thu Apr 11 18:20:27 2019 |
Valerian and Diego | OFFLINE | Software | CH2 | Timing issue between vamos and mugast |
A cut is seen on the TAC between MUGAST and the focal plane multiwire of VAMOS when one select XF or DC0_Y>-1500
Edit: This must be a reconstruction problem as it is not seen in the Raw files (using DC0_X for example)
Edit: This is not only a reconstruction problem as the cut appear again if one select DC0_Y
Edit: We changed VAMOS FAG validation window from 500ns to 800ns |
| Fixed | e744s |
Fri Apr 12 10:12:45 2019 |
Valerian | OFFLINE | Software | CH2 | Comparison between HF and CATS for ELab ThetaLab |
| Using the HF show noises that is not seen with CATS on the ToF spectra |
| Fixed | e744s |
Fri Apr 12 14:13:11 2019 |
Giuseppe D'Agata | OTHER | Software | N/A | Converted runs |
Runs additionally converted up to now:
70
71
80.0
80.1
81.0
81.1
82
83
84
85
86.1
91
94
95
96.1
97
98 |
| Fixed | e744s |
Fri Apr 12 19:44:09 2019 |
diego | VAMOS | Software | | SetAlias script for VAMOS identification |
|
| Fixed | e744s |
Fri Apr 12 22:44:43 2019 |
Valerian and Diego | OFFLINE | Software | CH2 | 13N measured in Vamos do correspond to protons events in MUST2 |
| Doing a cut on M vs M/Q corresponding to 13N one can see that most of the events do correspond to protons events in MUST2!!! |
| Fixed | e744s |
Sat Apr 13 00:27:08 2019 |
iulian nicolas Nikola Mariluz | RUN | Software | CH2 | Screenshots run119 v1 |
|
| Fixed | e744s |
Sat Apr 13 22:45:27 2019 |
Beyhan, Sylvain, Jaromir | AGATA | Software | N/A | Agata yellow phase 1 minute |
Agata yellow 1 minute
All the trigers emitted by (every) single crystal were refused by ACQ for 1 minute.
Reason unknown now. |
| Fixed | e744s |
Sat Apr 13 23:19:57 2019 |
Valerian, Freddy, Iulian and Fairouz | OFFLINE | Software | CH2 | Very preliminary results for two protons |
| Join are very preliminary spectra for the two protons events gated on 13N in VAMOS with a multiplicity 1 event in MUST2. This condition adds a lot of noise. |
| Fixed | e744s |
Sun Apr 14 12:11:52 2019 |
Valerian and Iulian | OFFLINE | Software | CH2 | VERY VERY preliminary results Gamma-p |
Around 8-10 events are found in the good energy vs Brho region and Si_T vs Si_E region for the gamma emission.
Joined are :
- the cut done for Energy vs Brho
- the "good" Events plotted on the Si_E vs Si_T spectra for each telescope.
one can see that most events are in, or close to the punch through but some of them ~8-10 are not -> very good candidates for proton after gamma emission |