Software and Computing
Vetting the ideal simulations for TPC alignment studies
I wanted to be sure that the simulations we're making for TPC alignment residual studies was really doing what we want it to do...
Log files have this output:
Alignment residuals with ideal alignment vers. 2
Now that we have figured out how to do simulations without hadronic processes (i.e.
NFit issue seen in emebedding QA, summary of issue
Speaker : Gene V. Buren ( BNL )
Talk time : 12:15, Duration : 00:20
Software and Computing Meeting
1-189, EVO, at 16:00 (GMT), duration : 01:00
Time | Talk | Presenter |
---|---|---|
12:00 | A review of recent changes in the ESL ( 00:15 ) 0 files | Levente Hajdu (BNL) |
12:15 | NFit issue seen in emebedding QA, summary of issue ( 00:20 ) 1 file | Gene V. Buren (BNL) |
12:35 | AOB ( 00:20 ) 0 files | All (All) |
Calibrations Meeting for Run 11
New York, at 19:30 (GMT), duration : 00:00
Run 11 pp 500GeV:
- TPC
- TOF
- BEMC/EEMC
Run 11 AuAu 19.6GeV:
- TPC
- TOF
- BEMC/EEMC
- FTPC
- PMD
Run 11 AuAu 200 GeV:
- TPC
- TOF
- BEMC/EEMC
- FTPC
- PMD
Software and Computing Phone Meeting
1-189, EVO, at 16:00 (GMT), duration : 01:00
Time | Talk | Presenter |
---|---|---|
12:00 | Embedding status ( 00:20 ) 1 file | Renee Fatemi (UKY) |
12:20 | AOB ( 00:20 ) 0 files | All (All) |
BeamLine for pp500 from HLT
The HLT group recorded BeamLine data during Run 11 pp500, which showed clear luminosity dependence.
How important is it for your job to check for disk space before dispatching them to the queue?
Zero mag field operation
Discussion points for taking zero field data to use in TPC alignment
Software and Computing Phone Meeting
1-189, EVO, at 16:00 (GMT), duration : 01:00
Time | Talk | Presenter |
---|---|---|
12:00 | Run 11 calibration status ( 00:20 ) 2 files | Grant Webb (UKY) |
12:20 | MC information on MuDst and vertex reconstruction efficiency ( 00:20 ) 0 files | Yuri Fisyak (BNL) |
12:40 | AOB ( 00:20 ) 0 files | All (All) |
Nfit vs. pT
One of the proposed effects contributing to RT ticket 2106 is that Nfit changes naturally as a function of pT, so coarse
Criteria for good primary vertices for Offline QA
In Offline QA at the moment, we restrict QA of tracks to those evens whose highest-ranked primary vertex passes two criteria:
Nfit vs. embedded mult
Following the RT ticket 2106 post from 2011-04-08 12:11:09 by Mustafa, I collected the relevant plots from 4 datasets:
Software and Computing Phone Meeting
1-189, EVO, at 16:00 (GMT), duration : 01:00
Time | Talk | Presenter |
---|---|---|
12:00 | VMC geometry, a closer look ( 00:20 ) 1 file | Jason Webb (BNL) |
12:20 | Embedding status, a focus on QM2011 ( 00:20 ) 2 files | Renee Fatemi, Terence Tarnowsky (UKY, MSU) |
12:40 | AOB ( 00:20 ) 0 files | All (All) |
RT Ticket 2103 : primaries
I repeated the exercise of matching tracks with new and old errors, as done in my previous blog post, but this t
Residuals from simulations with ideal alignment
Using simulations of pT = 5 GeV/c pi+ and pi- from Maxim, I tried to understand a little better what lead
Software and Computing Phone Meeting
1-189, EVO, at 16:00 (GMT), duration : 01:00
Time | Talk | Presenter |
---|---|---|
12:00 | Path forward for including Anti-particles in starsim ( 00:20 ) 0 files | Jason Webb (BNL) |
12:20 | Review of changes in TpcRS ( 00:15 ) 0 files | Yuri Fisyak (BNL) |
12:35 | Changes in the ESL ( 00:10 ) 2 files | Levente Hajdu (BNL) |
12:45 | AOB ( 00:15 ) 0 files | All (All) |
Issue 2106
For RT ticket 2106, there was some concern that the database updates between 20100821 and 20101213 might be somehow be re