Checking Function of FGT Event Display with current data
Here is a video of the Event Display in action.
Calibrations
Updated on Fri, 2013-03-08 12:18. Originally created by margetis on 2013-03-08 12:13.FGT Commissioning Meeting
Updated on Fri, 2013-03-08 15:47. Originally created by surrow on 2013-03-08 11:56.STAR Conference Room, at 20:00 (GMT), duration : 02:00
LINK TO: Commissioning plan
(1) Summary of commissioning activities / status : Bernd
Done:
- Documentation for shift crew (Mapping / Gas / HV)
- APV parameter scans
- HV scan data
- Pedestal stability vs. HV status
- Prepare new HV file to equalize response
- Take test run (Fri./Sat.) and interate at least once
- Switch to 6 time-bins next week on 03/15/13
- Request 15 time-bin operation for W trigger at the start of PHYSICS, i.e. between 03/08/13 and 03/15/13
- Participate in physics running with W trigger on 03/08/13 and with full trigger set on 03/15/13
- Experience at COMPASS / Thesis : Maxence
- Ramiro
(4) Switch to 6 time bins: Akio
EVO-------------------------------------------------------------------------------------------
People can connect via EVO (use the following link):
http://evo.caltech.edu/evoNext/koala.jnlp?meeting=MMMeMn292BDIDB9D9uD29
The password is fgtin2011
You can also connect via phone. Phone bridge numbers can be found at:
http://evo.caltech.edu/evoGate/Documentation/telephone.jsp
The meeting ID is 637 5313 and password 9215.
You can also connect via Skype by adding "evo.phone" (without the
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EVO-------------------------------------------------------------------------------------------
Stv TODO List
1. Stv is noy yet equipped to check is part of detector active or not.
FGT HV scan with day 065 and day 067
Use the data of day 65 and day 67 to get the cluster charge versus HV
FGT HV gain with day 065 data
With the following runs, we look the HV versus cluster charge with tracking from Akio's offline plots in the following link,
STAR heavy flavor and dilepton Moriond 2013
STAR heavy flavor and dilepton Moriond 2013 presentation 15+5
Some rough results from FGT APV tuning
We have collected data for several values of VFS
We now fit to Landau distribution shapes:
2006 EEMC Neutral Pions: New Mass Fitting (Near-final Run List)
NOTE: the trees were made with the wrong L2 thresholds and will need to be remade. Update following, shortly.
FGT Commissioning Meeting
Updated on Thu, 2013-03-07 16:00. Originally created by surrow on 2013-03-06 23:16.STAR Conference Room, at 20:00 (GMT), duration : 02:00
LINK TO: Commissioning plan
(1) Summary of commissioning activities
EVO-------------------------------------------------------------------------------------------
People can connect via EVO (use the following link):
http://evo.caltech.edu/evoNext/koala.jnlp?meeting=MMMeMn292BDIDB9D9uD29
The password is fgtin2011
You can also connect via phone. Phone bridge numbers can be found at:
http://evo.caltech.edu/evoGate/Documentation/telephone.jsp
The meeting ID is 637 5313 and password 9215.
You can also connect via Skype by adding "evo.phone" (without the
quotes) to your buddy list and calling that contact. Meeting ID and
password are the same as above.
EVO-------------------------------------------------------------------------------------------
A look at including anode voltage dependence for GridLeak with current calibrations
Missing tracks in current Stv
2013 BSMD Timing
I examined the files taken by Oleg Tsai
Runs14062066 onwards
Run Timing
x66 104/0
x67 104/5
x68 105/0
x69 105/5
x70 105/8
Run 9 200GeV Dijet Response Matrix Test II
Another look at the dijet response matrices ...
Old correction scheme had 4 bins based on detector eta topology and trigger content.