STAR Protected
Run 9 Data: Trigger Simulator Investigation
A look at the behavior of the trigger simulator (in data) as part of the investigation into raising the jet patch ADC thresholds in the simulation discussed here ...
HFT soft effort steering meeting
2014-09-18 15:00
2014-09-18 17:00
America/New York
Thursday, 18 September 2014
BNL 1-165, at 19:00 (GMT), duration : 02:00
BNL 1-165, at 19:00 (GMT), duration : 02:00
- Phone Bridge
ID: 1096183
EVO Phone Bridge Telephone Numbers:
---------------
- USA (BNL, Upton, NY)
+1 631 344 6100
- USA (Caltech, Pasadena, CA)
+1 626 395 2112
______________
ID: 1096183
EVO Phone Bridge Telephone Numbers:
---------------
- USA (BNL, Upton, NY)
+1 631 344 6100
- USA (Caltech, Pasadena, CA)
+1 626 395 2112
______________
| Time | Talk | Presenter |
|---|---|---|
| 14:00 | SSD geometry update ( 00:20 ) 1 file | jonathan |
| 14:20 | simulation without inner detectors ( 00:20 ) 1 file | jonathan |
STAR Management Meeting
2014-09-19 11:00
2014-09-19 12:30
America/New York
Friday, 19 September 2014
SeeVogh# 100 7671, BNL room 1-189, at 15:00 (GMT), duration : 01:30
SeeVogh# 100 7671, BNL room 1-189, at 15:00 (GMT), duration : 01:30
Agenda:
1) FMS preshower status (Oleg)
2) town Meeting Recap: cold/hot QCD
hotQCD and coldQCD jointly recommend
EIC as the highest priority for future
facility construction.
3) 2020+ forward upgrade plan/proposal
4) S&T review close-out
STAR dataset time from data-taken to publication
S&T committee is concerned about this.
Both Elke (spin) and I (HI/STAR) were asked to present this in
two different sessions.
Three action items:
I) HFT operation for next two runs
continue communications to DOE
ii) detail document of data-taking efficiency and improvements
(5 most important factors)
iii) detail (RCF) computing plan/optimization up to 2018
5) pA beam energy
should pA CM energy be same as pp or proton beam energies same?
1) FMS preshower status (Oleg)
2) town Meeting Recap: cold/hot QCD
hotQCD and coldQCD jointly recommend
EIC as the highest priority for future
facility construction.
3) 2020+ forward upgrade plan/proposal
4) S&T review close-out
STAR dataset time from data-taken to publication
S&T committee is concerned about this.
Both Elke (spin) and I (HI/STAR) were asked to present this in
two different sessions.
Three action items:
I) HFT operation for next two runs
continue communications to DOE
ii) detail document of data-taking efficiency and improvements
(5 most important factors)
iii) detail (RCF) computing plan/optimization up to 2018
5) pA beam energy
should pA CM energy be same as pp or proton beam energies same?
Discrepancy between data and MC in background estimation -- II
We have noted that the discrepancy between data and embedding has lumnosity dependence.
2013 - Barrel Noise Study - Difference in Pedestals
Difference in Pedestals calculated and plotted
Fluxes 2013 pp510, 2014 AuAu200, 2014 He3Au200, 2014 pAu200, 2014 pp200, and 2014 pp510 collision.
I have created a table with R and Z distribution for flux of neutrons, charged hadrons, electrons and gammas for diffrent collision for STAR geometries 2013 and 2014.
EEMC Cal Run9-09-16-2014
Different landau fitting:
Above: [0]*TMath::Landau(x,[1],[2],0)+[3] Below: landau(3)
Introduction for heavy flavor D meson
1.MC simulation
We use Pythia 8 to simulate Heavy Flavor D meson.
Code example: /star/u/amcw7777/pwg/MCProduction/Produce/starsim.C
Geometry tag: y2014a
< Run12 Trigger Simulator Test
Picked out one run 13108057 with JP0 prescale equal to 1 and trying to plot the maxiaml jet patch ADC (from 18 jet patches) on the left, the barrel trigger patch adc in the middle and the differ
Run-11 Transverse Jets: Revisiting Cuts
As we move toward a final result, I estimate the following as the list of necessary tasks:
Pion-kaon femtoscopy in Au+Au collisions at STAR - Hot Quarks 2014
Data analysed:
BES: 7.7GeV, 19.6GeV, 39GeV
130GeV