STAR Protected
Cluster energy fraction in 0.7 radius: detector eta > 1.5
Energy fraction in NxN cluster within r=0.7 radius: detector eta < 1.5
Figure 1a: 2x1/0.7 energy fraction [number of counts per given fraction]
Cluster energy fraction in 0.7 radius: detector eta < 1.5
Energy fraction in NxN cluster within r=0.7 radius: detector eta < 1.5
Figure 1a: 2x1/0.7 energy fraction [number of counts per given fraction]
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
2008.11.18 Cluster isolation cuts: 2x1 vs. 2x2 vs. 3x3
Ilya Selyuzhenkov November 18, 2008
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 |
Expected Resource needs from STAR Operations for Upgrades in FY09
Updated on Thu, 2008-11-13 21:16. Originally created by xzb on 2008-11-13 21:16.Speaker : Zhangbu Xu ( BNL )
Talk time : 09:00, Duration : 00:20
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 R&D and Capital Funds - All
2) Report from the Shifts Committee - Olga
3) Run8 p+p data production status - Bedanga/Jerome
4) Progress with the difficult manuscripts – Helen and Jamie
5) Rotation of PWG conveners: UPC and HF - All
6) QM09 abstract deadline for PWG: 1st Dec. - Bedanga
* --===================================--*
Brief Summary:
1) Attending: Bill, Zhangbu, Jamie, Nu, Olga, Bedanga
2) Rotation of PWG conveners: UPC and HF: Nu discussed with Janet (UPC) and Manuel& Alex.
Janet: agreed to proceed. She will provide the list of the active members soon.
Manuel: agreed to proceed. More discussion between Nu and Alex on when to happen. Alex already send in a list of the active members.
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
FUSE & SSHFS - Overview and example in STAR online environment
FUSE (Filesystem in Userspace)
Panic Talk on Eta An (2)
Panic Talk On Eta Transverse Single Spin Asymmetry at very forward angles.
The current draft of my contribution to Panic Proceedings is panic08WritupDraft5.pdf
Fixing Slave Replication In A STAR Offline Database Mirror
Mike's trick for fixing an offline database slave when it won't sync with the master is to be carried out as follows:
cd /var/run/mysqld
ls -lh | grep "mysqld-relay-bin"
11 Nov
November 2008 posts
(No) multiplicity bias in Au+Au + trigger
The figure below shows the refmult distribution for events with a central trigger (run-4 central data, triugger 15105) and various high-pt trigger particle selections (>2 GeV, >4 GeV and >