STAR Protected
D0 Signal Update-Comparison of HPSS and NFS files
Analysis of HPSS and NFS files for D0 signal
iSCSI SAN Speed Test Results
The hardware used for testing is as follows:
-iSCSI SAN:
Search for QCD Critical Point: High Moment of Event by Event Multiplicity Distribution
Updated on Mon, 2009-11-30 00:58 by luoxf. Originally created by dongx on 2009-09-28 18:14.Reference
Speaker : Xiaofeng Luo ( LBNL/USTC )
Talk time : 11:40, Duration : 00:20
FHC cosmic ray test
Updated on Tue, 2009-10-06 22:01 by xuanli. Originally created by dongx on 2009-09-28 18:11.Reference
Speaker : Xuan Li ( Shandong Univ. )
Talk time : 10:10, Duration : 00:20
STAR Management Meeting
EVO: Title: STAR Management Meeting // Community: STAR // Password: star // Phone Bridge: +1 626 395 2112 (CA) / +1 631 344 6100 (NY) // ID: 1269411 // Password: 0952, at 15:00 (GMT), duration : 01:00
Time: 11 AM - 12 PM EDT
* --===================================================================--*
Agenda:
1) STAR Collaboration preparation - Bedanga
2) Run10 shift and QA board - Olga
* --====================================================================--*
Brief Summary:
0) Attendency:
1)
Notes:
1) STAR TPC Review (key= star2009), June 4,5, BNL. Ron Settler (chair). Review report.
2) NPE Committee, H. Huang (chair)
3) STAR TOF Close Out Review, Aug. 10-11. Review report and The Plan.
4) STAR FMS Review agenda, Sept. 1-2, BNL, P. Jacobs (chair). Review report
Future Meetings:
1) SQM2009: Sept. 27-Oct. 2, Buzios, Brazil
2) STAR Collaboration meeting, Oct. 5-10, Berkeley
3) DNP 2009, Oct. 13 - 17, Waikoloa
4) STAR-DoE HFT CD-1 review, postpond to Nov., BNL
5) APS April meeting, Feb. 13-17, 2010, Washongton DC. (abstract deadline: Oct. 23, 2009)
Reproducing a rough estimate.
An email contained the following notes from Bill Christie regarding the BHT3 cross section, and I want to reproduce this logic to
Preliminary examination of -/+ in st_W production
I grabbed the files of electron candidate tracks from Matt Walker which he used for his 10 Electron E/p from pp500 L2W events from the st_W sample production,
Run6 Transverse Data Energy Dependent Mass Shift Analysis
Here we take a look at the run6 transverse DATA, to better understand the energy dependent gain correction.
1. FPD at middle position (Xoffset~30.7cm)
Rates in different bXing subsets
Following from the previous blog post, I investigated the rates in each of the three regions.
bXing plots for vernier scans.
I broke down the vernier scan run 10097097 by bunch crossing using mudst->event()->l0Trigger().bunchCrossingId7bit(mRunNo) , incrementing the histogram for every patch that's above