Ralph test area
Updated on Thu, 2006-06-15 15:08. Originally created by rlbrown on 2006-06-15 15:08. Under:This is my first test page.
XML Geometry demonstration
Updated on Wed, 2006-06-14 11:50. Originally created by testadmin on 2006-06-14 10:52.Speaker : Maxim Potekhin ( BNL )
Talk time : 12:50, Duration : 00:10
Library readiness for SVT+SSD+Vertex
Updated on Wed, 2006-06-14 10:51. Originally created by testadmin on 2006-06-14 10:51.Speaker : Lidia Didenko ( BNL )
Talk time : 12:40, Duration : 00:10
B-EMC calibration status and revised agenda
Updated on Wed, 2006-06-14 11:21. Originally created by kocolosk on 2006-06-14 10:49.Speaker : Adam Kocoloski ( MIT )
Talk time : 12:20, Duration : 00:10
- SMD/PSD pedestals (Priscilla Kurnadi, UCLA) Propose to set pedestal = 0 for problematic channels so we can go back and analyze these in greater detail with muDsts. Should be < 10% of channels. Priscilla has analyzed the stability of pedestals; final determination of number of tables to upload still needs to be made. Estimate to production-ready: 3 weeks.
- BTOW status (Dave Staszak, UCLA) Dave S. is using Dave Relyea's code to produce status tables using fastOffline muDst's. He has been on this project for ~2 weeks and we expect to show first status table and pedestal calculations for a single run at next EMC phone. Estimate to production-ready: 4 weeks. Will need more time than that to finish status tables, but I think we can produce a set that accounts for the majority of problems in that time frame
- BTOW peds The online pedestals should not be used. Several channels have unphysical widths. Options for replacing these peds include: a) Jan's L2 peds, b) pedestals returned from the status tables, or c) separate analysis. So, estimate: <= 4 weeks, shorter if L2 pedestals are deemed adequate.
E-EMC status and timeline for readiness for Y6 p+p
Updated on Wed, 2006-06-14 10:51. Originally created by testadmin on 2006-06-14 10:49.Speaker : Jan Balewski (TBC) ( IUCF )
Talk time : 12:30, Duration : 00:10
This talk was not confirmed.
The Effects of the Inclusion of SVT Hits in the Reconstruction of K0Shorts
Updated on Wed, 2006-06-14 10:40. Originally created by testadmin on 2006-06-14 10:38.Speaker : Anthony Timmins ( BHAM )
Talk time : 12:10, Duration : 00:10
QA on the new productions of CuCu @ 200 GeV
Updated on Wed, 2006-06-14 10:38. Originally created by testadmin on 2006-06-14 10:35.Speaker : Christine Nattrass ( Yale )
Talk time : 12:00, Duration : 00:10
StEmcTriggerMaker
Updated on Fri, 2007-10-19 12:29. Originally created by kocolosk on 2006-06-13 15:34. Under: Documentation provided by Renee Fatemi
MOTIVATION:
MOTIVATION:
First Iteration
Updated on Thu, 2007-10-18 13:59. Originally created by kocolosk on 2006-06-12 22:04. Under: March 27, 2007
Software
Updated on Fri, 2007-10-19 11:47. Originally created by kocolosk on 2006-06-12 21:36. Under:The main EMC offline reconstruction chain consists of:
pp2006: transverse polarization
Updated on Mon, 2006-06-12 14:21. Originally created by genevb on 2006-06-12 13:59. Under: Just as was done in the pp2006: longitudinal polarization,
I calibrated using the technique described SpaceCharge and GridLeak Calibration How-To Guide. Just a
couple notes:
Here are the plots and output from my final iterative pass:
- I did not even attempt to look at the no-calibration data as the pp2006: longitudinal polarization showed this to be of little help. I simply assumed that ZDC east+west would again be the best relevant scaler.
- Again, calibration was done without the beamline constraint with one exception. For the last pass, I used the values predicted by all the previous passes along with the beamline constraint. The result was a new data point which sits almost exactly on the fit curves, not changing the fits, which is good evidence that the fit had indeed converged.
- The fits for the offset parameter were not as good as the other fits, but almost certainly good enough to move forward.
- Spread in the measures of the SpaceCharge ionization did not improve in any significant way with the use of the beamline calibration. This implies that either the beamline calibration is not doing anything useful, or the spread in the sDCA distribution is dominated by something else.
Here are the plots and output from my final iterative pass:
* Constraint on SC x GL = 7.32e-07
* Guesses on SC = 8.73e-08 , 4.39e-08 , 8.63e-08 , 4.39e-08
* Guesses on GL = 8.39 , 11.3 , 8.48 , 11.3
* Guesses on SO = 3.27e+04 , 3.26e+04
*** FINAL CALIBRATION VALUES: ***
SC = 8.63e-08 * ((zdce+zdcw) - (3.27e+04)) with GL = 8.48
Database load balancer, status and next step
Updated on Wed, 2006-06-07 12:21. Originally created by testadmin on 2006-06-07 10:42.Speaker : Mike DePhillips ( BNL )
Talk time : 13:00, Duration : 00:10
AOB
Updated on Wed, 2006-06-07 10:42. Originally created by testadmin on 2006-06-07 10:37.Speaker : All ( All )
Talk time : 12:50, Duration : 00:10
Xrootd status and recent developments
Updated on Wed, 2006-06-07 10:59. Originally created by pjakl on 2006-06-07 10:34.Speaker : Pavel Jakl ( NPI-AS )
Talk time : 12:30, Duration : 00:10
Additional link to plots:
http://www.star.bnl.gov/~pjakl/xrootdStat/index.html
Simulation, new SVT review request
Updated on Wed, 2006-06-07 10:34. Originally created by testadmin on 2006-06-07 10:33.Speaker : Maxim Potekhin ( BNL )
Talk time : 12:20, Duration : 00:10
Cu+Cu 200 GeV possible issues
Updated on Wed, 2006-06-07 10:33. Originally created by testadmin on 2006-06-07 10:32.Speaker : Yuri Fisyak ( BNL )
Talk time : 12:10, Duration : 00:10
Year6 p+p (TPC) calibration status
Updated on Wed, 2006-06-07 11:02. Originally created by testadmin on 2006-06-07 10:31.Speaker : Gene Van Buren ( BNL )
Talk time : 12:00, Duration : 00:10
BeamLine Constraint
- Data from days 73-130 processed (includes first longitudinal polarization period,
and transverse polarization period, but not second longitudinal period).
- Studied and verified validity of triggers I used.
- Identified some problem fills, like:
- Fill 7697 (day 93): removing some of the data makes point drop back down; will use
calib from previous fill - Fill 7712 (day 97): that's all the statistics we have; will use
calib from next fill - Fill 7786 (day 117): two independent subsets of the data show similar calibs;
will use the calib found for that fill
- Fill 7697 (day 93): removing some of the data makes point drop back down; will use
- Discussed volatility during transverse running with a RHIC operator,
seems not unexpected. - Processing of other May longitudinal data progress.
SpaceCharge & GridLeak
- Calibrations using the May longitudinal polarization dataset is done (without using
BeamLine Constraint) and is in the DB.
More details are available pp2006: longitudinal polarization. - Distortion is so large without any calibration that tracking is being affected
(tracks are being split at the gap between inner and outer TPC sectors). - Performed checks that BeamLine Constraint does not affect SpaceCharge calibrations,
and that SpaceCharge does not affect BeamLine calibration. - Very close to finishing transverse polarization calibration (one more iteration).
- Will need to re-calibrate with different beam polarizations/energies
Short in TPC IFC East
- As You do not have access to view this node, there is a distortion due to an
electrical short in the TPC IFC East - Excess current continues to rise and has exceeded the amount which can be
explained by bridging a 2 MOhm resistance gap, which most probably isolates it
to one of the patched 3 MOhm resistance gaps. - Jim Thomas and I have discussed how to handle this varying distortion and
will work on implementing it in the coming weeks. - Distortion is not large enough to prevent moving forward with a dEdx calibration.
Gene Van Buren
gene@bnl.gov
Review charges reminder, logistic
Updated on Tue, 2006-06-06 12:57. Originally created by jlauret on 2006-06-06 12:50.Speaker : Myself ( BNL )
Talk time : 17:00, Duration : 00:10
Dear STAR Collaborators, The email concerns an upcoming planning exercise related to STAR's inner tracking detectors. The review, which will take place just before the Collaboration meeting (July 7-8) at BNL, will place particular emphasis on understanding how a plan which optimizes our physics program in the next few years (including planned upgrades of STAR's capability) informs the question of future utilization of the SVT and when it should be taken out of the STAR set-up. The draft charge for the SVT Review Committee is attached below. The agenda and the membership of the review panel will be announced in the coming week. As a final comment, I would like to thank, in advance, Jerome Lauret, and Spiros Margetis for organizing the necessary effort for this review, as well as all the members of the STAR software and SVT analysis teams who have been working steadily behind the scenes for close to a year now to produce the necessary understanding to inform this important discussion. Sincerely, Tim HallmanCharge to the SVT Review Panel: The charge to the committee is to comment on how a plan which optimizes the scientific output of the STAR Collaboration in the next 3-5 years influences the issue of whether and when the STAR Silicon Vertex Tracker should be removed.
The core physics goals of the STAR Collaboration in the next 3-5 years include:
Planned analysis and who is going to make presentations
Updated on Tue, 2006-06-06 14:03. Originally created by jlauret on 2006-06-06 09:37.Speaker : All ( All )
Talk time : 17:20, Duration : 00:30
Comments / questions:
Data set status and location summary
Updated on Tue, 2006-06-06 12:49. Originally created by didenko on 2006-06-06 09:32.Speaker : Lidia Didenko ( BNL )
Talk time : 17:10, Duration : 00:10