antiproton in Au+Au 200GeV Run14
Updated on Wed, 2017-06-21 00:24 by zhux. Originally created by llope on 2017-05-26 18:23.proton in Au+Au 200GeV Run14
Updated on Fri, 2017-06-16 04:12 by zhux. Originally created by llope on 2017-05-26 18:22.Please find the bad run lists attached for Run 14. Please do not embed into those runs.
Particle: proton and anti-proton
Number of events: 500k each
Real Data: Au+Au 200GeV Run14
Centrality: 0-10% central collisions based on refmult
Triggers: 450050, 450060, 450005 , 450015, 450025
Production chain: P16id + NoPxlIT, NoIstIT, NoSstIT
Library: SL16d
Vz: (-6, 6) cm.
Phi: (0, 6.29) in radian flat
Rapidity: (-1, 1) flat
pT: (0, 3) GeV flat
Number of particles per event: To be discussed with the embedding expert
Request ID | 20172102 |
Priority: EC | 0 |
Priority: pwg | Normal |
Status | Larger (or full) sample done, producing PWG QA [6/7] |
Physics Working Group | Bulk correlations |
Requested by | llope |
Contact email(s) | roliesha@physics.ucla.edu |
Contact phone(s) | |
PWG email(s) | bulkcorr-hn@www.star.bnl.gov |
Assigned Deputy: | Not assigned |
Assigned Helper: | Not assigned |
Request type: | Standard Embedding request (particle in real events) |
Number of events | 500000 = 500 K |
Magnetic Field | ---- SELECT MAGFIELD ---- |
Collision Type | auau 200GeV |
Centrality | ---- SELECT CENTRALITY ---- |
BFC tags | P16id, +, NoPxlIT, NoIstIT, NoSstIT |
Production | ---- SELECT PRODUCTION TAG ---- |
Geometry: simu | ---- SELECT GEOMETRY ---- |
Geometry: reco | ---- SELECT GEOMETRY ---- |
Library | ---- SELECT STAR LIBRARY ---- |
Vertex option | ---- SELECT VERTEX OPTION ---- |
Pileup option | No |
Detector Set | Triggers: 450050, 450060, 450005 , 450015, 450025 |
File lookup |
Particle | Alpha |
Particle settings | dalitz |
Particles per event | 1 |
Vertex Z, cm | -30 < Vertex < 30 |
Gaussian sigma in X,Y,Z (cm), if applicable | 0, 0, 0 |
Vertex offset: x, mm | 0 |
Vertex offset: y, mm | 0 |
Φ (phi), radian | 0 < Φ < 6.29 |
η (eta) | -0.5 < η < 0.5 |
Pt, GeV | 0 < Pt < 30 |
Xi(1530) - Richard Witt
Updated on Fri, 2017-05-26 13:52. Originally created by tlusty on 2017-05-26 13:52.Productions: P11idAuAu200 and P12idpp200
pt type: flat
pt range: 0.0 to 6.0 (to allow for pt skewing)
eta range -1.5 to 1.5 (though 1.2 to 1.2 is probably sufficient)
primary vertex Z: -50 to +50
I need at least 100k in each multiplicity bin (and for the p+p by
itself). With a reasonable estimate of 2% efficiency that should give
me ~200 reconstructed Xi0(1530)'s in the lowest pt bins for each
multiplicity.
Request ID | 20172101 |
Priority: EC | 0 |
Priority: pwg | Normal |
Status | New |
Physics Working Group | LFS-UPC |
Requested by | tlusty |
Contact email(s) | tlusty@gmail.com |
Contact phone(s) | |
PWG email(s) | lfsupc-hn@www.star.bnl.gov |
Assigned Deputy: | Not assigned |
Assigned Helper: | Not assigned |
File lookup |
Particle | Alpha |
Particle settings | dalitz |
Particles per event | 1 |
Vertex Z, cm | -30 < Vertex < 30 |
Gaussian sigma in X,Y,Z (cm), if applicable | 0, 0, 0 |
Vertex offset: x, mm | 0 |
Vertex offset: y, mm | 0 |
Φ (phi), radian | 0 < Φ < 6.29 |
η (eta) | -0.5 < η < 0.5 |
Pt, GeV | 0 < Pt < 30 |
May 2017, Collaboration Meeting, BNL
Updated on Fri, 2017-05-26 11:02. Originally created by nihar on 2017-05-26 11:02.
Trigger bias for IFF 500 (kinematics)
Updated on Fri, 2017-05-26 10:36. Originally created by avossen on 2017-05-26 10:22.BES event plane correlations
Updated on Thu, 2017-05-25 18:04. Originally created by iupsal on 2017-05-25 12:50.Presentation of first and second order event plane correlations.
Y->ee in AuAu14, nSigE cut efficiency
Updated on Thu, 2017-05-25 09:34. Originally created by matonoli on 2017-05-25 09:34.Summary of nSigmaElectron cut efficiency determination for Upsilon->ee analysis in BHT2 AuAu 2014.
FMS Timing Misc Investigations
Updated on Wed, 2017-05-24 22:58. Originally created by bsumma on 2017-05-24 22:58.
Wilga2017 v2
Updated on Wed, 2017-05-24 16:24. Originally created by siejka on 2017-05-24 16:24.Wilga2017 v2
The 2th test results for the MWPC with new pad plane design
Updated on Wed, 2017-05-24 08:52. Originally created by shenfw on 2017-05-24 08:49.
Draft for WPCF2017
Updated on Wed, 2017-05-31 04:03. Originally created by tnonaka on 2017-05-23 19:45.
Collaboration Meeting Slides
Updated on Tue, 2017-05-23 11:01. Originally created by dolv719 on 2017-05-23 11:01.
Distance between proton and pion, electron and pion prediction for different methods : I70, Ifit and dmdx
Updated on Tue, 2017-05-23 10:37. Originally created by fisyak on 2017-05-23 10:37.
Analysis Note for D_TT
Updated on Tue, 2018-06-12 02:02. Originally created by jcmei on 2017-05-23 09:27.Analysis note for 2012 Lambda D_TT.
Please check the most updated version in the attachments.
Paper Proposal: Run 9 pp200 Forward Di-jet Asymmetry
Title: Longitudinal Double-Spin Asymmetries for Di-jet Production at intermediate pseudorapidity in Polarized $pp$ Collisions at $\sqrt{
run progress / AuAu 53 GeV preparation
Updated on Mon, 2017-05-22 11:51. Originally created by jhlee on 2017-05-22 11:51.AuAu at 53 GeV projection for e+e-
Updated on Mon, 2017-05-22 11:55 by jhlee. Originally created by syang on 2017-05-22 09:49.Speaker : Shuai
Talk time : 13:30, Duration : 00:20
Trigger Board Meeting for Run17
Updated on Mon, 2017-05-22 08:53. Originally created by jhlee on 2017-05-22 08:46. 2017-05-22 13:00
America/New York
Monday, 22 May 2017
BNL Physics 1-224 and SeeVogh (ID 102 1767), at 17:00 (GMT), duration : 00:00
BNL Physics 1-224 and SeeVogh (ID 102 1767), at 17:00 (GMT), duration : 00:00
- Run progress
- AuAu 53 GeV preparation
- AuAu 53 GeV projection
- AuAu 53 GeV preparation
- AuAu 53 GeV projection
Time | Talk | Presenter |
---|---|---|
13:00 | run progress / AuAu 53 GeV preparation ( 00:30 ) 1 file | |
13:30 | AuAu at 53 GeV projection for e+e- ( 00:20 ) 2 files | Shuai |
Tracking performance check on Yuri's VMC production
Updated on Fri, 2017-06-02 16:58. Originally created by dongx on 2017-05-18 18:47.In effort of pursuing to set up the HFT embedding infrastructure, Yuri did some development using VMC geometry. These are some first cosmic ray samples produced:
The Lambda filter used in the MC sample production
Updated on Thu, 2017-05-18 00:19. Originally created by jcmei on 2017-05-18 00:18.The Lambda filter is used in the new generation of MC sample in order to improve the efficiency and save the space of disk.
The filter is based on the StMCFIlter.