Yield vs. NxN cluster energy fraction in r=0.7
Yield vs. NxN cluster energy fraction in r=0.7
Figure 1c: 2x1/0.7 ratio
Efficiency vs. NxN cluster energy fraction in r=0.7
Efficiency vs. NxN cluster energy fraction in r=0.7
Figure 1b: 2x1/0.7 ratio
Energy fraction in NxN cluster within r=0.7 radius
Energy fraction in NxN cluster within r=0.7 radius
Figure 1a: 2x1/0.7 ratio
2009 algo upgrade 1
Updated on Sun, 2008-12-07 22:42. Originally created by balewski on 2008-11-18 09:59. Under:The following deficit of the CVS version of PPV have been corrected for in December of 2008
2008.11.18 Cluster isolation cuts: 2x1 vs. 2x2 vs. 3x3
Ilya Selyuzhenkov November 18, 2008
QA for Au+Au 200GeV run 7 - Multiplicity vs. Vz
Updated on Tue, 2008-11-18 02:31. Originally created by kikola on 2008-11-18 02:31.QA - Stability of Multiplicity vs. Vz
Mapping DB Proposal
Updated on Mon, 2008-11-17 21:24. Originally created by kocolosk on 2008-11-17 21:23. Under:Proposal
We propose to add a new set of tables to the Calibrations_emc database that will track the electronics mapping for the BEMC, BSMD, and BPRS and allow for an alterna
QM09 Abstract
Updated on Mon, 2008-11-17 13:12. Originally created by bbiritz on 2008-11-17 13:12.Hi All,
Calculation of the efficiency of D0 with pT
Updated on Tue, 2009-06-09 14:43. Originally created by jai2006 on 2008-11-17 10:39.A hand calculation of the D0 efficiency with increasing pT is studied here.
11 BPRS absolute gains from MIP, ver1.0 ( example of towers)
Updated on Tue, 2009-03-10 14:43. Originally created by mattheww on 2008-11-17 09:31. Under:BPRS absolute gains from MIP, v
STAR Management Meeting
BNL, 50-I-189, at 15:00 (GMT), duration : 01:00
Conference Phone Number: 510 486 7333
Time: 10 - 11 am EDT
* --===================================--*
Agenda:
1) FY09 Capital and R&D proposals to be submitted to ADBoard - Nu
2) Updated report from the Shifts Committee - Olga
3) Review Committee for FHC - Nu
4) AoB
* --===================================--*
Brief Summary:
1) Attending: Helen, Olga, Jamie, Zhangbu, Nu, Bernd, Bill
2) Shift Committee: action items (a) send the satistics to Council; (b) ask Council discuss how to respons to those institutes who did not fulfile their shift responsibles - -ask for explainations; reduce number of authors or sign up more shifts early in next run;
3) CAD meeting (Bill/Jamie): Cool down on Feb. 2nd; No more access after Feb. 6th; Feb. 20: collisions for physics. STAR needs a list of priorities, starts the discussions in PWGc; for example, Spin: (i) first W+ cross section at mid-y; (ii) hadron-jet correlation; (iii) ALL
4) Funding:send the existing both lists to ADBoard for discussions of the priorities
5) Online tracking: group forming
Notes:
1) STAR Regional meeting at VECC: Nov. 24 - 25
2) QM09 abstract deadline: Dec. 15th
3) BES meeting: Dec. 17-18 at BNL: summarise goals and next steps in BES
| Time | Talk | Presenter |
|---|---|---|
| 10:00 | Shift Assignments ( 00:20 ) 1 file | Olga |
02 BTOW swaps ver=1.3
Updated on Sun, 2008-11-16 21:13. Originally created by balewski on 2008-11-16 20:12. Under:Example of MIP peak for BTOW towers pointed by TPC MIP track: 
Spectra for 4800 towers (raw &
BEMC + EEMC Online Plots
Updated on Mon, 2009-02-16 13:00. Originally created by gdwebb on 2008-11-16 17:18.When considering the modification of the current online PPlots we have the following goals:
new IST code
Updated on Fri, 2008-11-21 08:28. Originally created by bouchet on 2008-11-16 10:01.I run the bfc chain with the new version of StiIstDetectorBuilder from
current note
Updated on Tue, 2008-12-23 16:30. Originally created by bouchet on 2008-11-15 17:59.current version of the note on SSD efficencies during CuCu run V (work with Vi Nham Tram)
11/29 : update
Potential distortions at projected luminosities for different species
Updated on Fri, 2009-05-29 21:57. Originally created by genevb on 2008-11-14 19:38. Under:Here I show the expected distortions in the STAR TPC as represented by the pointing error of tracks to the primary vertex (otherwise known as the DCA) due to experienced (star symbols) and projecte
W Simulations
Updated on Fri, 2008-11-14 16:48. Originally created by seelej on 2008-11-14 16:48.I produced some initial simulations for the W+- studies in the barrel. The MuDst are located in
/star/institutions/mit/seelek/Wsims/
Minutes/Action Items
Updated on Fri, 2008-11-14 15:14. Originally created by margetis on 2008-11-14 15:14.Reference
Talk time : 13:32, Duration : 00:20
Action Items:
1) Jonathan to check Willie's fixes for UPG15 and prepare instructions
2) Data Set Production for LBL Workshop(?where? BNL/PDSF?)
Efficiency calculation for new StiIstDetectorBuilder
Updated on Fri, 2008-11-14 13:52. Originally created by wleight on 2008-11-14 13:52.The below plots were generated from 1000 single-pion events, using a version of the StiIstDetectorBuilder that treats each IST ladder as one big wafer (as was done for all previous IST geometries).
pi0 paper discussion log1
Updated on Fri, 2008-11-14 12:03. Originally created by yoo on 2008-11-14 11:52.Hi all,