| Status |
ExpNbr |
Date |
Author |
Type |
Category |
Target-Source |
Subject |
| Fixed | com2019 |
Fri Apr 5 11:26:09 2019 |
Adrien, Freddy and the world | OFFLINE | General | N/A | Mask reconstruction CATS1-CATS2 run 223 |
Mask between CATS1 and CATS2 in Z=-2190 Reconsctruction with nptool and attached mugast.detector and ConfigCATS.dat attached.
The beam seems to be shifted strongly to the [B]left[/B] of the beam line during the run. not clear yet if the shift of the mask is due to :
- shift of cats
- shift of the mask itself
|
| Attachment 1: MaskCATS1CATS2_run223.pdf
|
|
| Attachment 2: mugast.detector
|
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
Target
THICKNESS= 9.7 micrometer
ANGLE= 0 deg
RADIUS= 24 mm
MATERIAL= CD2
X= 0 mm
Y= 0 mm
Z= 0 mm
% CATS POSITION centered, slightly WRONG
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
CATSDetector
X1_Y1= 35.56 -35.56 -2658 mm
X28_Y28= -35.56 35.56 -2658 mm
X1_Y28= 35.56 35.56 -2658 mm
X28_Y1= -35.56 -35.56 -2658 mm
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
CATSDetector
X28_Y1= -35.56 35.56 -2045 mm
X1_Y28= 35.56 -35.56 -2045 mm
X28_Y28= -35.56 -35.56 -2045 mm
X1_Y1= 35.56 35.56 -2045 mm
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%%% Telescope 1 %%%%%%%
M2Telescope
X128_Y128= 115.88 9.61 154.54 mm
X128_Y1= 104.8 101.89 125.09 mm
X1_Y1= 14.55 102.4 160.63 mm
X1_Y128= 25.63 10.12 190.08 mm
SI= 1.00
SILI= 0.00
CSI= 1.00
VIS= all
%%%%%%% Telescope 2 %%%%%%%
M2Telescope
X128_Y128= -11.23 102.42 160.87 mm
X128_Y1= -101.39 102.39 124.37 mm
X1_Y1= -113.17 10.36 153.56 mm
X1_Y128= -23.03 10.38 190.05 mm
SI= 1.00
SILI= 0.00
CSI= 1.00
VIS= all
%%%%%%% Telescope 3 %%%%%%%
M2Telescope
X128_Y128= -113.28 -12.52 153.32 mm
X128_Y1= -101.58 -104.77 124.82 mm
X1_Y1= -11.39 -104.58 161.48 mm
X1_Y128= -23.1 -12.34 189.98 mm
SI= 1.00
SILI= 0.00
CSI= 1.00
VIS= all
%%%%%%% Telescope 4 %%%%%%%
M2Telescope
X128_Y128= 13.82 -104.92 160.72 mm
X128_Y1= 104.3 -104.95 125.08 mm
X1_Y1= 115.75 -12.73 153.76 mm
X1_Y128= 25.23 -12.65 189.43 mm
SI= 1.00
SILI= 0.00
CSI= 1.00
VIS= all
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
Mugast Trapezoid
DetectorNumber= 7
X128_Y128= 40.99 21.69 -98.21 mm
X1_Y128= 23.34 39.63 -98.04 mm
X1_Y1= 57.53 120.53 -32.58 mm
X128_Y1= 122.2 55.73 -32.67 mm
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
Mugast Trapezoid
DetectorNumber= 3
X128_Y128= -48.05 -23.23 -95.05 mm
X1_Y128= -24.83 -39.35 -99.33 mm
X1_Y1= -58.24 -119.46 -32.57 mm
X128_Y1= -122.86 -54.55 -32.41 mm
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
Mugast Trapezoid
DetectorNumber= 1
X128_Y128= -23.05 42.83 -99.66 mm
X1_Y128= -40.74 25.21 -99.65 mm
X1_Y1= -120.65 58.67 -32.39 mm
X128_Y1= -55.66 123.17 -32.55 mm
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
Mugast Trapezoid
DetectorNumber= 5
X128_Y128= 21.68 -41.48 -100.19 mm
X1_Y128= 39.55 -23.81 -100.11 mm
X1_Y1= 119.55 -57.08 -33.23 mm
X128_Y1= 54.81 -121.7 -33.12 mm
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
Mugast Trapezoid
DetectorNumber= 4
X128_Y128= -15.11 -44.73 -99.25 mm
X1_Y128= 10.11 -44.71 -99.35 mm
X1_Y1= 43.37 -125.07 -32.74 mm
X128_Y1= -48.18 -125.07 -32.45 mm
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
Mugast Square
DetectorNumber= 10
X128_Y128= 111.36 97.74 89.82 mm
X1_Y128= 147.47 9.83 90 mm
X1_Y1= 147.7 9.88 -1.79 mm
X128_Y1= 111.63 97.7 -2.02 mm
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
Mugast Square
DetectorNumber= 9
X128_Y128= 107.49 -95.88 0.0 mm
X1_Y128= 143.81 -8.21 0.0 mm
X1_Y1= 143.81 -8.21 91.7 mm
X128_Y1= 107.49 -95.88 91.7 mm
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
Mugast Annular
DetectorNumber= 11
Center= -0.3 1 -126.9 mm
ModularLeaf
DefaultValue= -5000
Leafs= GATCONF_MASTER GATCONF_SLAVE1 GATCONF_SLAVE2 CONFDEC_AGATA CONFDEC_VAMOS DATATRIG_CATS1 DATATRIG_CATS2 TMG_MUGAST_HF TCATS_MUGAST_HF TVAMOS_MUGAST_HF EVAMOS_AGATA ECATS_AGATA E_AGATA
X= TMG_MUGAST_HF TMG_MUGAST_HF TCATS_MUGAST_HF EVAMOS_AGATA EVAMOS_AGATA ECATS_AGATA
Y= TVAMOS_MUGAST_HF TCATS_MUGAST_HF TVAMOS_MUGAST_HF E_AGATA ECATS_AGATA E_AGATA
% Leafs=
% X=
% Y=
|
| Attachment 3: ConfigCATS.dat
|
ConfigCATS
ZPROJ -2190
% RECONSTRUCTION METHOD
% 5 recosntructions are available :
% FSECH : for fitted hyperbolic secante method
% ASECH : for analytic hyperbolic secante method
% AGAUSS : for analytic Gaussian method
% CENTROIDE : for a simple centroide method
RECONSTRUCTION_METHOD CATS1X ASECH
RECONSTRUCTION_METHOD CATS1Y ASECH
RECONSTRUCTION_METHOD CATS2X ASECH
RECONSTRUCTION_METHOD CATS2Y ASECH
% INVERSION CATS2 11 and 12 inversed
%DISABLE_CHANNEL CATS2STRX27
% CORRECTION (Correction3Points or Correction4Points : depends on the reconstruction method)
% use Correction3Points for GAUSS, SECH or BAR3
% use Correction4Points for BAR4
% CORRECTION_METHOD CATS1X Correction4Points
% CORRECTION_METHOD CATS1Y Correction4Points
% CORRECTION_METHOD CATS2X Correction4Points
% CORRECTION_METHOD CATS2Y Correction4Points
% CORRECTION COEF
% See TCATSPhyscis.cxx to see the correction formula where the coefficient of correction is applied.
% CORRECTION_COEF CATS1X 0.60
% CORRECTION_COEF CATS1Y 0.60
% CORRECTION_COEF CATS2X 0.60
% CORRECTION_COEF CATS2Y 0.60
SHIFT_CATS CATS1X 0
SHIFT_CATS CATS1Y 0
SHIFT_CATS CATS2X 0
SHIFT_CATS CATS2Y 0
|
| Fixed | e793s |
Fri Mar 19 09:54:58 2021 |
Adrien, Freddy and Franco | GRIT | General | 3-alpha | Alpha calibration and noise on MG3 and MG4 after the experiment |
While starting the alpha source runs after the experiment we found unexpected noise on MG3 and MG4 which cannot be excluded just by masking some Y mates (The X mates were already masked for both of them). We cannot figure out the origin of this noise.
Run 652 and 653 -> alpha runs without pedestal suppression
Run 655 -> alpha run during the night with pedestal suppression. Here MG3 and MG4 are not in the trigger.
Run 658 -> alpha run after an attempt to mask some noisy strips. The number of ORD is anyway high (some 10^4) but we see some alphas on MG3 and MG4.
Run 660 -> same as 658 but with higher thresholds on X (8250) and Y (7600 on MG3 and 7950 on MG4) to write less on disk but actually nothing changes. Therefore we are writing about 2.7 GB per hour.
The other runs (654, 656, 657 and 659) can be discarded. |
| Fixed | com2019 |
Fri Apr 5 23:19:04 2019 |
Adrien et Valerian | OFFLINE | General | CD2 | Experimental Kinematic Line from dp |
We used run 253 to obtain a convincing Kine line and Ex spectrum at backward angle.
Stat is still limited but the distribution is convincing. |
| Attachment 1: Kine253.pdf
|
|
| Pinned | com2019 |
Fri Apr 5 23:34:46 2019 |
Adrien et Valerian | OFFLINE | General | N/A | Converting data and adding stat to Kine Plot |
Here is a procedure to convert a run and add data the Kinematic plot.
Every 4Go there will be a file change, convert the file and add it to the chain using the following step:
Step O: Take your favorite ortholinear keyboard
Step 1: Login in the right environment
- open a terminal from one of the mugast computer
- type lpcgrit to login to lpcgrit and source the right environmt
- you should see red lpcgrit invite of command
Step 2: Convert the file using the offline program
This Convert the file from the ganil .dat file and contained only MUGAST and CATS stuff
- type npp MUGAST/offline in the terminal to reach the correct folder
- ./Offline run_com2019/run_0ZZZ-DD-MM-YY.HHhMMmSSs root_com2019/run_ZZZ_0.root
- OR
- ./Offline run_com2019/run_0ZZZ-DD-MM-YY.HHhMMmSSs.R root_com2019/run_ZZZ_R.root
Step 3: Analyse the file using the npanalysis program
This could be used with any file, either from Offline conversion, or the VAMOS Analysis conversion or the Merged Tree from AGATA.
- type npp MUGAST in the terminal to reach the correct folder
there is an error below caused by the ortholinear keyboard, I guess, corrected using a normal keyboard:
- npanalysis -D mugast.detector -C Calibration.txt -E ./Reaction/16Odp.reaction -T offline/root_com2019/run_0253.root AutoTree -O PhyZZZ.root
- The run will be created in the NPOutputs/ folder
Step 4: Add the file to the KineMacro
- vim macros/Kine.cxx
- Add the new file in the LoadChain method
- root macros/Kine.cxx
- Enjoy the soothing feeling of a smooth knematic line during a late night shift.
|
| Fixed | TEST |
Thu Mar 21 10:37:47 2019 |
Adrien and Valerian | MUST2 | General | N/A | Test TOF must2 |
To make sure the mate work correctly we took an alpha run with a delayed fag on the MUVI stop:
- all mate register a time in the the middle of the range as expected (fag delayed by 350ns, range is 600ns)
Test with time calibrator, all channel are enable, pulser on channel 3 of each mate T1X:
- energy spectrum: pulser where we expect it.
- we expect to see a time calibrator spectrum on channel 3 of each mate. instead we see times spectrum on Channel 3 of mate 1 and 2, channel 12 of mate 1, channel 14 of mate2. nothing else
Conclusion
The problem was that the synctst had to be checked and ord unchecked |
| Attachment 1: Time_behavior_withDAS.png
|
|
| Fixed | e744s |
Thu Apr 11 10:38:13 2019 |
Adrien and Valerian | BEAM | General | N/A | They are preparing 14O beam |
News from (edit after talking to Pierre D.)
- They are preparing the 14O beam.
- We should have 14O at moderate intensity early afternoon.
- The beam should be at full intensity inG1 around 21h-23h.
- Run end Wenesday 18h sharp
- Omar is on call at any time
|
| Fixed | e793s |
Mon Feb 8 11:25:29 2021 |
Adrien and Freddy | S1 | General | N/A | FSC run |
we ran FSC on all card. S1 is dismounted.
Pulser goes on all channel and works well so electronic is fine.
We will ask Laurent to remount the detector and re run the test. |
| Attachment 1: fscE_08022023.png
|
|
| Attachment 2: fscT_08022022.png
|
|
| Fixed | TEST |
Fri Jan 18 15:32:50 2019 |
Adrien Valérian | GRIT | General | N/A | Calimero tests Muvi2 MM7 MG10C |
After disabling nptool Multithreading, online is working fine again.
Concerning Calimero, it is currently working both on MUVI1 and MUVI2 for the X at least.
Joined here is the result of Calimero for MG10C on MUVI2 channel 3 (MM7). |
| Attachment 1: Calimero_MUVI2_MM7_allchannels_allmates__stat100000_withchannelsenabled.png
|
|
| Attachment 2: Calimero_MUVI2_MM7_allchannels_allmates_withchannelsenabled.png
|
|
| Fixed | e744s |
Tue Apr 9 15:48:00 2019 |
Adrien Valerian | OFFLINE | General | CD2 | Expected gamma background in coincidence with proton in MUST2 |
This is a plot of the Gamma in AGATA in coincidence with proton in MUST2 for the entire run 256.
It gives a hint of the expected gamma background due to fusion evaporation for the upcoming experiment looking for a bump around 3.5 MeV
The proton are selected only with the E-DE plot, so not in coinc with proton stopping in the first stage. |
| Attachment 1: Gamma_Forward_Proton.png
|
|
| Fixed | e744s |
Sat Apr 13 21:34:02 2019 |
Adrien Matta -> update Iulian | RUN | General | N/A | Inconsistent info in the run message-fix explained in reply |
Be careful to fill in correctly all info in the start run message.
There is inconsistency in run 121 comment (target 2) and list (target 3).
Thèse information will be used for the analysis.
Iulian->
This discrepancy has been addressed |
| Fixed | TEST |
Fri Dec 14 09:08:46 2018 |
Adrien Matta | OTHER | Social | N/A | Test Post |
| MUGAST ELOG is now ONLINE |
| Fixed | TEST |
Sat Mar 23 15:26:06 2019 |
Adrien Matta | OTHER | Software | N/A | To do list |
FSC:
- Autoconf programme to set all regular parameter (PAC gain, TAC range, ORD, no mask, no pulser)
Sentinel:
- Making the program
- Preparing start script
- Preparing stop script
- Preparing init script
Online/offline:
- Look into ZMQ to replace GRU
- Datum through zmq
- Switch NPSpectraServer/Client to ZMQ and datum
- CsI Calibration with db scan
- 3-alpha calibration using NPCalibration
HV:
- Remote read
- Auto logging
- Alert on trip
- Bt/HV/sector on/off
|
| Fixed | com2019 |
Sun Mar 31 18:11:28 2019 |
Adrien Matta | OTHER | General | N/A | To do list for the commissioning (please edit!) |
Here is a to do list of thing we should do ahead of the commissioning. Please self assigned task by putting your name next to it. Don't hesitate to ask for help, or clarification or anything you might need.
Timing:
We need to established the timing for CATS and MUST2 and prepare the inspection line to be able to check it during beam time (NO ONE ATTRIBUTED)
[X] CATS signal will come from the CATS crate into a FIFO (CATS FIFO) in the MUGAST NIM bin, from there it is distributed to the TAC and the GMT
(Beyhan, Neils, François)
[X] Add inspection line from the FAG and the CATS FIFO with cables of the same length to the patch panel
(Ruxandra, Nicolas, Freddy)
[X] Calculate the 16O beam speed: yyy mm/ns
6 MeV/A => v= 3.38734 cm/ns
- Provide the CATS1/2 to target length (mécanic or surveyor): xxx mm
- The TOF of the beam from CATS1 To target is: ZZZ ns
- The TOF of the beam from CATS2 To target is: ZZZ ns
- Send a pulser to SYNTEST on MUST2 and CATS and measured the electronic delay between the two
- Add the physical delay and check the signal are aligned in G1
- Check the signal are aligned outside the room (any joke with patch panel cable being of different length
 )
- Label the patch panel, we will need to adjust this timing at the beginning of the exeperiment
Do the same for the VAMOS/ MUST2 timing (NO ONE ATTRIBUTED)
Analysis:
Prepare macro for near line analysis: (Padova group) [X]
- 4 panels (d,p): ELab:ThetaLab, Ex with relevant 017 states indicated,Ex-Edc plot, Edc with relevant 017 gammas indicated
- 4 panels (d,d)/(p,p): ELab:ThetaLab, Ex with relevant 016 states indicated,Ex-Edc plot, Edc with relevant 016 gammas indicated
- 4 panels (d,t): ELab:ThetaLab, Ex with relevant 015 states indicated,Ex-Edc plot, Edc with relevant 015 gammas indicated
*** Prepare level scheme with gamma rays for (d,p)17O (d,t)15O and (d,d)16O. Add Sn and Sp, add them to the blog and print them (Cyril Lenain started)
Add agata/vamos branches to MUGAST project (Freddy)
MUGAST :
Do a time calibrator in running conditions with 20-30 ns delay between start and stop (A.Matta/V Alcindor)
- take data: DONE
- analyse them and add calibration to the analysis.
|
| Pinned | com2019 |
Mon Apr 1 11:02:00 2019 |
Adrien Matta | MUST2 | Hardware | N/A | Switching on and off LV/HV for MUST2 crate |
HVM group could be used to switch on and off the LV and HV for the MUST2 crate.
The command could be lauched from the analysis environment: start a terminal and type:
> lpcgrit
This will connect to lpcgrit and source the correct environment.
Be careful: HV on mugast should not be on when the BT are off, this could damaged the PAC:
- Power up sequence : switch on BT first, then HV
- Power down sequence :Switch off HV first, then BT.
To switch on group use:
> hvm_group <group name> <on|off>
The following group exist:
- BT-MGA -> Low voltage for GRIT trapezoid and annular detector
- BT-MGB -> Low voltage for GRIT trapezoid
- BT-MUST -> Low voltage for MUST2 and 90 deg
- HV-MG -> GRIT Trap and Annular HV
- HV-MUST -> MUST2 Si and CsI HV
The programme return only once the voltage finished ramping up, so be patient. Once the voltage are set, it will print-out the relevant channel. If a channel trip, the programm print out the status of all the channel.
NB: over voltage on +5V channel is "normal" and ignored as an error by the program
To check the status of the voltage crate use the hvm_print command:
to print VAMOS and MUST2:
> hvm_print
to print MUST2:
> hvm_print MUST2
to print VAMOS:
> hvm_print VAMOS
|
| Fixed | com2019 |
Wed Apr 3 11:03:53 2019 |
Adrien Matta | CATS | Hardware | N/A | Cats mask will be shifted |
The propulsif supporting the cats mask is leaking.
It will be tighten to fix the leak, this lead to a small shift toward the left of the beam when looking at vamos. |
| Fixed | com2019 |
Wed Apr 3 11:05:36 2019 |
Adrien Matta | DAQ | Software | N/A | MFM scaler reading |
| MfM scaler are read correctly for Must2 U2M but output some -1 for the numexo2 integrated scaler. |
| Fixed | com2019 |
Sat Apr 6 08:38:51 2019 |
Adrien Matta | OFFLINE | General | CD2 | We see d,3he more than d,t at forward angle |
We see more (d.3he) than dt
there seems to be another reaction going up to 40deg Lab |
| Attachment 1: Kine256_0-256_3.pdf
|
|
| Fixed | com2019 |
Sat Apr 6 10:09:53 2019 |
Adrien Matta | OFFLINE | General | CD2 | We see d,4He |
| Adrien Matta wrote: | We see more (d.3he) than dt
there seems to be another reaction going up to 40deg Lab |
The line at 40 deg matched 16O(d,4He)14N g.s. |
| Fixed | e744s |
Sat Apr 13 12:04:56 2019 |
Adrien Matta | OTHER | Social | N/A | Blow some steam this afternoon (staturday13th) |
If some of you want to blow some steam this afternoon Crossfit Caen ( located in Mondeville, you. Can find them on google map) is organising an initiation Wod this afternoon for their 4th anniversary. Here is the program of the day:
Les quatre ans de la boxe commence, on vous attend avec impatience et venez nombreux. 👌🏻💪🏻 Si vous voulez découvrir le Crossfit ou tout simplement essayer (wod initiation),ça sera avec plaisir ! 😁
4 ans de CrossfitCaen 🔥🔥
Le déroulement de la journée !! 👌🏻
10h-13h Floater 1
10h30 Wod Team 20 personnes
11h15 Initiation
12h Wod Élite
12h30 Wod Indiv
13h30 Kids
14h-17h Floater 2
14h15 Wod Indiv
15h Initiation
15h45 Wod Élite
16h30 Wod Team
20h Tenue Correcte Exigée |
| Ongoing | e744s |
Sat Apr 13 21:57:48 2019 |
Adrien Matta | RUN | General | N/A | Inconsistent info in the run message |
| Adrien Matta wrote: | Be careful to fill in correctly all info in the start run message.
There is inconsistency in run 121 comment (target 2) and list (target 3).
Thèse information will be used for the analysis. |
--> Well.. in entry 4175 it is written target 3...
... ... |