Heavy Flavor
Updated on Fri, 2009-09-25 12:16. Originally created by sowinski on 2009-09-25 12:16.Time | Talk | Presenter |
---|---|---|
14:00 | NPE analysis in run 2008 p+p ( 00:30 ) 1 file | Wei Xie (Purdue Univ.) |
14:30 | NPE analysis in run 2005/6 p+p ( 00:30 ) 1 file | Shingo Sakai (UCLA) |
15:00 | NPE analysis with TOF in 2008 p+p ( 00:30 ) 1 file | Fu Jin (SINAP) |
15:30 | Coffee Break ( 00:15 ) | |
15:45 | NPE analysis in run 8 d+Au ( 00:30 ) 1 file | Xin Li (Purdue Univ.) |
16:15 | NPE analysis in run 2008 d+Au ( 00:30 ) 1 file | Wenqin Xu (UCLA) |
16:45 | NPE analysis in CuCu 2005 ( 00:45 ) 1 file | Anders Knospe (Yale Univ.) |
17:30 | NPE analysis discussion ( 00:30 ) 0 files | All (all) |
LIght Flavor Spectra PWG
Updated on Fri, 2009-09-25 12:11. Originally created by sowinski on 2009-09-25 12:11.HFT Software
Updated on Fri, 2009-09-25 11:22. Originally created by margetis on 2009-09-25 11:22. 2009-09-25 13:30
Etc/GMT-5
Friday, 25 September 2009
510-4867333, at 17:30 (GMT), duration : 00:00
510-4867333, at 17:30 (GMT), duration : 00:00
Here
Embedding activities and status
Updated on Fri, 2009-10-09 08:12 by rfatemi. Originally created by jeromel on 2009-09-25 09:08.Reference
Speaker : Renee Fatemi ( UKY )
Talk time : 10:10, Duration : 00:20
Online tracking for High Level Trigger in STAR
Updated on Fri, 2009-10-09 00:44 by sss. Originally created by jeromel on 2009-09-25 08:56.Reference
Speaker : Xiangming Sun ( LBNL )
Talk time : 12:40, Duration : 00:20
Grid and network tuning activities
Updated on Fri, 2009-10-09 12:56 by olson. Originally created by jeromel on 2009-09-25 08:55.Reference
Speaker : Doug Olson ( LBNL )
Talk time : 12:20, Duration : 00:20
KISTI facility readiness, a status report
Updated on Tue, 2009-10-06 09:11. Originally created by jeromel on 2009-09-25 08:44.Reference
Speaker : Jerome Lauret ( BNL )
Talk time : 12:00, Duration : 00:20
Multi-source data access and movement
Updated on Fri, 2009-10-09 09:06 by zer0. Originally created by jeromel on 2009-09-25 08:40.Reference
Speaker : Michal Zerola ( NPI/ASCR )
Talk time : 11:40, Duration : 00:20
Computing activities overview
Updated on Fri, 2009-10-09 13:43. Originally created by jeromel on 2009-09-25 08:38.Reference
Speaker : Jerome Lauret ( BNL )
Talk time : 10:50, Duration : 00:30
Database activities and performance tuning
Updated on Tue, 2009-10-06 16:44 by testadmin. Originally created by jeromel on 2009-09-25 08:37.Reference
Speaker : Dmitry Arkhipkin ( BNL )
Talk time : 11:20, Duration : 00:20
h-/h+ Update and Calibration Readiness for Run 9 Processing
Updated on Fri, 2009-10-09 11:11 by genevb. Originally created by jeromel on 2009-09-25 08:35.Reference
Speaker : Gene Van Buren ( BNL )
Talk time : 09:40, Duration : 00:30
Coffee break
Updated on Fri, 2009-09-25 09:09. Originally created by jeromel on 2009-09-25 08:33.Reference
Talk time : 10:30, Duration : 00:20
E/BEMC GEANT geometry study and reshape
Updated on Fri, 2009-10-09 08:52 by jwebb. Originally created by jeromel on 2009-09-25 08:30.Changes have recently been made to the EEMC and BEMC geometries in starsim in order to (1) better reproduce the calorimeters as built, and (2) in the EEMC resolve a long standing issue with the sam
Reference
Speaker : Jason C. Webb ( Valparaiso )
Talk time : 09:20, Duration : 00:20
TOF progress and readiness
Updated on Fri, 2009-10-09 02:02 by geurts. Originally created by jeromel on 2009-09-25 08:27.Reference
Speaker : Frank Geurts ( Rice )
Talk time : 09:00, Duration : 00:20
BNL-PDSF transfer, Sept. 2009
Updated on Thu, 2009-09-24 18:03. Originally created by andrewar on 2009-09-24 17:31.We updated the transfer proceedure to make use of the OSG automated monitoring tools. Perviously, the transfers ran between stargrid04 and one of the NERSC data transfer nodes.
Charge Sign Ratio for pp500 SL09b production
Previously Jan showed a plot (figure 10) of the charge seperated W yields. The pl
Spin PWG Presentation W Analysis (9/24/2009)
Updated on Thu, 2009-09-24 10:35. Originally created by seelej on 2009-09-23 23:06.FHC pythia mini-bias simulation for Lambda
I use the pythia mini-bias codes to study to look for the lambda decay products energy deposit in FHC with Lambda->n+pi0.
More?
Updated on Wed, 2009-09-23 17:18. Originally created by matis on 2009-09-23 17:18.Talk time : 11:40, Duration : 00:20