EPD 2018 - First dark current checks
Updated on Mon, 2018-02-26 10:21. Originally created by rjreed on 2018-02-04 12:17.A crew working on 4 Feb 2018:
dAu embedding request
Updated on Fri, 2018-02-02 14:16. Originally created by lkramarik on 2018-02-02 14:16.Standard Embedding request (particle in real events)
pAu embedding
Updated on Fri, 2018-02-02 14:13. Originally created by lkramarik on 2018-02-02 14:10.For pAu, two embeddings are needed for two production streams.
The PicoDst format
"For many years, the data flow model in HEP has been
FEE box NW filled
Updated on Sun, 2018-02-04 17:33. Originally created by lisa on 2018-02-01 23:59. The EPD FEE box on the NW corner of STAR has been filled. In my opinion, it has a real beauty and serious economy of space. The fibers have room to gently bend, and there is no strain
Update 02.01.2018 -- Run 9 Purity
Continuing with the study of the gamma-rich purity in run 9 pp, I've checked the purity with a tighter zTtrk cut.
topological distributions for signal and background
Updated on Thu, 2018-02-01 22:31. Originally created by xgn1992 on 2018-02-01 18:42.This is using the data-driven simulation for the signal and background study.
EPD, ETOF, ...
Updated on Thu, 2018-02-01 14:00. Originally created by jwebb on 2018-02-01 14:00.Reference
Talk time : 17:00, Duration : 00:20
- EPD
- Review nearly done... code in reasonable shape before collaboration meeting, after geometry and utility methods decoupled from data objects.
1M more events for Lambda in Au+Au 200GeV run-11 0-80%
Updated on Sun, 2018-03-04 00:17 by zhux. Originally created by llope on 2018-02-01 13:51.1M more events for AntiLambda in Au+Au 200GeV run-11 0-80%
Updated on Sun, 2018-03-04 00:16 by zhux. Originally created by llope on 2018-02-01 13:46.The previous request is here:
https://drupal.star.bnl.gov/STAR/starsimrequests/2017/jul/20/antilambda-auau-200gev-run-11-0-80
Run numbers to use for this request are listed below.
................................................................................................................................................................
AntiLambda in Au+Au 200GeV run-11 0-80%
Original request (followed below by additional information):
Particle: Lambda (& Lambda_bar)
Au+Au@200GeV
Run11
production: P11id
Trigger Setup: AuAu200_production_2011
minimum bias
Trigger Id: 350003, 350013, 350023, 350033, 350043
0.2 GeV < pT < 5.0 GeV (flat)
|y_lambda| < 0.5
0 < phi < 2pi
V_z < 30cm, V_r < 2cm, V_z - V_z(VPD) < 3cm
Centrality Defn: RefMult3
1 lambda per event
500K events
Additional Information:
1. Centrality from 80-100% is not needed. 0-5% to 70-80% is good (9 bins).
But if you think still this is too much, at least I need the most two central bins (0-5% & 5 -10%).
Boundaries :
refmult[9] = {10,22,43,76,125,193,281,396,466}
refmult3[9] = {16,34,67,120,196,301,440,618,725}
2. How about 5% of refmult embedded particles per event?
3. Run numbers (previous request):
[12133002 - 12133061] - good
[12129011 - 12129029] - good
[12127002 - 12127051] - good
...Run numbers (present request) :
12132009,
12134006,
12135012,
12136007,
12167046,
12170058,
12171015
12132009,
12134006,
12135012,
12136007,
12167046,
12170058,
12171015
4. Mag Field : RFF
5. I’m currently doing my analysis in the range of 0.2 GeV/c < pT < 2.0 GeV/c. But, Since Xianglei’s trees has the option of going up to 5GeV, I thought it would be an advantage to have a wide range incase if I happen to re-do the analysis in higher pT bin (2.0 < pT < 5.0). However, If it is too much open, then go for 0.2 GeV/c < pT < 2.0 GeV/c.
Request ID | 20180508 |
Priority: EC | 0 |
Priority: pwg | High |
Status | Larger (or full) sample done, producing PWG QA [6/7] |
Physics Working Group | Bulk correlations |
Requested by | llope |
Contact email(s) | wjllope@wayne.edu,nalinda05kl@gmail.com |
Contact phone(s) | 313-577-9805 |
PWG email(s) | bulkcorr-hn@www.star.bnl.gov |
Assigned Deputy: | Not assigned |
Assigned Helper: | Not assigned |
File lookup | &nbsp;&nbsp;<span style="-webkit-text-stroke-width: initial; font-size: 14px; -webkit-text-stroke-color: rgb(0, 0, 0); font-family: Helvetica;">Run numbers :&nbsp;</span><span class="Apple-tab-span" style="font-family: Helvetica; font-size: 14px; white-space: pre; -webkit-text-stroke-width: initial; -webkit-text-stroke-color: rgb(0, 0, 0);"> </span><span style="-webkit-text-stroke-width: initial; font-size: 14px; -webkit-text-stroke-color: rgb(0, 0, 0); font-family: Helvetica;">[12133002 - 12133061] - good</span> <div style="font-family: Helvetica; font-size: 12px;"><span style="-webkit-text-stroke-color: rgb(0, 0, 0); -webkit-text-stroke-width: initial; font-size: 14px;"><span class="Apple-tab-span" style="white-space: pre;"> </span>&nbsp; &nbsp; &nbsp;<span class="Apple-tab-span" style="white-space: pre;"> </span>[12129011 - 12129029] - good</span></div> <div style="font-family: Helvetica; font-size: 12px;"><span style="-webkit-text-stroke-color: rgb(0, 0, 0); -webkit-text-stroke-width: initial; font-size: 14px;"><span class="Apple-tab-span" style="white-space: pre;"> </span>[12127002 - 12127051] - good</span></div> <div><span style="-webkit-text-stroke-color: rgb(0, 0, 0); -webkit-text-stroke-width: initial; font-size: 14px;"><br /> </span></div> |
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 |
HFT Embedding
Updated on Thu, 2018-02-01 15:41. Originally created by jwebb on 2018-02-01 13:13.Reference
Talk time : 16:40, Duration : 00:20
- Hijing + zerobias events (one run, 10 files) submitted and running. Expect jobs to complete next week.
Update on Optimization
Updated on Thu, 2018-02-01 13:06. Originally created by jwebb on 2018-02-01 13:06.iTPC Software Readiness / Review
Updated on Thu, 2018-02-01 14:53 by perev. Originally created by jwebb on 2018-02-01 12:57.Reference
Speaker : Victor
Talk time : 16:00, Duration : 00:20
https://drupal.star.bnl.gov/STAR/blog/perev/stica-itpc-mrging
S&C Offline Software
Updated on Thu, 2018-02-01 12:54. Originally created by jwebb on 2018-02-01 12:54. 2018-02-01 16:00
2018-02-01 17:00
America/New York
Thursday, 1 February 2018
1-189, SRN, at 21:00 (GMT), duration : 01:00
1-189, SRN, at 21:00 (GMT), duration : 01:00
SRN 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 |
---|---|---|
16:00 | iTPC Software Readiness / Review ( 00:20 ) 0 files | Victor |
16:20 | Update on Optimization ( 00:20 ) 0 files | Dmitri |
16:40 | HFT Embedding ( 00:20 ) 0 files | |
17:00 | EPD, ETOF, ... ( 00:20 ) 0 files |
Weekly Meeting (Feb. 1)
- Chong: brief update for pi0 calibration
- David: Second look at MIPs in the FMS
StiCA + iTPC mrging
Updated on Wed, 2019-04-03 11:33. Originally created by perev on 2018-02-01 12:17. Tue Apr 2
=======
Angle dependency for 15+ tracks
.png)
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Angle dependency for 15+ tracks
.png)
Report on TOP/BOTTON Difference in FMS Run 15
Updated on Thu, 2018-02-15 11:49. Originally created by heppel on 2018-02-01 11:47.
Sampled (Np,Npbar), 3 runs of 1M events each, AuAu 7.7
Updated on Tue, 2018-03-27 22:38 by zhux. Originally created by llope on 2018-02-01 10:43.This is needed to support a QM talk
Details here:
https://drupal.star.bnl.gov/STAR/system/files/tnonaka_embedding_request_summary.pdf
This request is described on page 8 of this pdf.
Note it is a series of three 1M event embeddings runs. In this case, the number of embedded protons and
antiprotons are to be obtained from sampling from provided histograms. Number of events
needed is 1M for 0-5%, 1M for 5-10%, and 1M for 10-15% centrality based on refmult3.
additional details (bad run list, pt slope, etc) may be found in files on the rcf
with paths provided by the pdf linked to above
Note 1M events for each of these three centralities is larger than the number of
real events available. Real events will be repeated. Please try to use as many
real events as possible to limit reuse.
Request ID | 20180507 |
Priority: EC | 0 |
Priority: pwg | High |
Status | Larger (or full) sample done, producing PWG QA [6/7] |
Physics Working Group | Bulk correlations |
Requested by | llope |
Contact email(s) | wjllope@wayne.edu |
Contact phone(s) | 3135779805 |
PWG email(s) | bulkcorr-hn@www.star.bnl.gov |
Assigned Deputy: | Not assigned |
Assigned Helper: | Not assigned |
File lookup | &amp;nbsp; |
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 |
Fixed (Np,Npbar), 25 runs of 100k events each, AuAu 200 run10
Updated on Sun, 2018-03-25 22:41 by zhux. Originally created by llope on 2018-02-01 10:35.This embedding is needed to support a QM talk.
Details here:
https://drupal.star.bnl.gov/STAR/system/files/tnonaka_embedding_request_summary.pdf
This request is described on page 7 of this pdf.
Note it is a series of 100k embeddings runs where the number of protons and
number of antiprotons is fixed.
additional details (bad run list, pt slope, etc) may be found in files on the rcf
with paths provided by the pdf linked to above
NOTE: This request supercedes Request ID: 20174903
Request ID | 20180506 |
Priority: EC | 0 |
Priority: pwg | High |
Status | Larger (or full) sample done, producing PWG QA [6/7] |
Physics Working Group | Bulk correlations |
Requested by | llope |
Contact email(s) | wjllope@wayne.edu |
Contact phone(s) | 3135779805 |
PWG email(s) | bulkcorr-hn@www.star.bnl.gov |
Assigned Deputy: | Not assigned |
Assigned Helper: | Not assigned |
File lookup | &amp;nbsp; |
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 |
Update 01.31.2018 -- Run 9 pp: Underlying Event Study
An open question with regards to the "Uncorrelated Jets" method of approximating the underlying event is how to normalize the uncorrelated jet distribution (if at all).