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HF PWG meeting 20160602

Run-11 Transverse Jets: Fine Bins vs. Single Bin

I updated the background correction for high-pT.

J/Psi mass from toy simulation

Reconstructed J/Psi mass peak from electron-positron pairs in the FMS

PYTHIA subprocesses:

  • 86 g+g->J/Psi+g

Jet Mini Workshop

2016-05-27 12:00
2016-05-27 17:00
America/New York
Friday, 27 May 2016
Online, at 16:00 (GMT), duration : 05:00
TimeTalkPresenter
12:00Underlying Event Studies ( 00:20 ) 0 filesGrant Webb
12:30Underlying event studies ( 00:20 ) 0 filesLi Yi
13:00Underlying event in non-boost invariant systems ( 00:20 ) 0 filesZilong Chang
13:30Break ( 01:00 ) 0 files
14:30Mixed Event Method ( 00:20 ) 1 fileAlex Schmah
15:00Unfolding Algorithms and Instrumental Corrections ( 00:20 ) 0 filesGrant for Brian Page
15:30Unfolding (AA) ( 00:20 ) 1 fileJan Rusnak

Postshower design

Postshower with two halves and top trapezoidal section.
The edges are projected from the shower max position in the center of the inner- and outermost towers in the FMS.

MTD local meeting 20160526

 

Global Lambda Polarization PRL (Lisa, Upsal, Voloshin 2016)

1 April 2017 - Response to referee and editor comments and manuscript revis

MTD local meeting 20160512

 

Run 16 notes

 5/12/2016

Investigation of what dAu rates can be run:
Comparing a standard auau HFT run with the test 70 kHz dAu zdc rate

IWND2016

 

pp@500GeV long range small Delta phi correlations

Supplemented material:

1. Embeded whole pythia event in ZeroBias real data. (Thanks to Zilong!)

D0 Run14 P16id Production

Statistics as presented in Frank Guert's talk at the PAC meeting (https

BUR1718 - HFT Preliminary and other open charm results

 2016/05/04  v1:  edited section 1.1 "Progress on physics analyses with the HFT", put

NPE v2 in Au+Au 200, 62.4 and 39 GeV run 10: v2 results with low-purity bins removed

Analysis code for UPC picoDST (Krakow format)

Analysis code for UPC picoDST (Krakow format)

PicoDst QA Run16065027 (test)

 

QA for D mesons in pp200 run 15

QA for D mesons in pp200 run 15

A look on Run16 Au+Au 200 GeV space charge

Lumonisity has been kept approximately constant throughout fills in run16. We were wondering if the space charge has a strong intensity depedence. 

April 2016

STAR Newsletter

April 2016 edition

HF PWG meeting 20160331