SDCC Announcements
Updated on Mon, 2020-11-30 11:28. Originally created by dongx on 2020-11-30 11:28.Reference
Speaker : Jeff Landgraf ( BNL )
Talk time : 12:00, Duration : 00:05
Pi/K/p spectra in isobar collisions
Updated on Mon, 2020-11-30 10:48. Originally created by yali on 2020-11-30 10:48.Reference
Speaker : Yang Li ( University of Science and Technology of China )
Talk time : 10:00, Duration : 00:20
TPC weekly
2020-12-02 15:00
America/New York
Wednesday, 2 December 2020
virtual , at 20:00 (GMT), duration : 00:00
virtual , at 20:00 (GMT), duration : 00:00
Minutes:
Tim reported on Gating Grid status
Crate has all modified modules. It was tested locally.
The web based script by Tonko does not seem to work after the upgrades. He is aware of it.
The polarity is swtiched at the connector for all.
The sector 8 is special and should be checked.
FV will contact David on the slow control of the gating grid; how should it be implemented?
Alexei has been working on laser system
- optics replaced; signal looks good
- started with alignment of akll rafters
- propbably will need another week
Software
- no discussion as some key people could not join the meeting today. There was a longer discussion on the run-19 alignment at the monthly S&C meeting
- It is of high priority to get this resolved; will have as agenda point next week
Flemming Videbaek is inviting you to a scheduled ZoomGov meeting.
Topic: TPC weekly
Time: Dec 2, 2020 03:00 PM Eastern Time (US and Canada)
Join ZoomGov Meeting
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DAEHEP_2020_PRELIMINARY_FIGURES
Updated on Sun, 2020-12-06 20:05. Originally created by apandav on 2020-11-29 02:45.
UrQMD 3GeV pileup study
Updated on Sat, 2020-11-28 16:48. Originally created by yuzhang1 on 2020-11-28 16:48.
Tracking Efficiency Uncertainty meeting
2020-12-02 10:00
2020-12-02 12:00
America/New York
Wednesday, 2 December 2020
https://cesnet.zoom.us/j/3472866, at 15:00 (GMT), duration : 02:00
https://cesnet.zoom.us/j/3472866, at 15:00 (GMT), duration : 02:00
| Time | Talk | Presenter |
|---|---|---|
| 10:00 | Tracking Efficiency Uncertainty (known issues) ( 00:20 ) 1 file | Yuri Fisyak |
| 10:20 | Previous eff. studies ( 00:20 ) 1 file |
Tracking Efficiency Uncertainty
Tracking Efficiency Uncertainty tak force page
17.11.2020, The charges to the task force
Data table problem for GPC#94
Updated on Thu, 2020-11-26 23:49. Originally created by xgou on 2020-11-26 23:49.
Data table problem for GPC#94
Updated on Thu, 2020-11-26 23:48. Originally created by xgou on 2020-11-26 23:48.
STAR PWGC meeting
Updated on Fri, 2020-12-18 14:34. Originally created by marr on 2020-11-25 17:31. 2020-12-18 09:30
America/New York
Friday, 18 December 2020
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 14:30 (GMT), duration : 00:00
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 14:30 (GMT), duration : 00:00
1) Paper preview: Di-pi^0 correlations in p+p, p+Al, and p+Au collisions at sqrt{s_NN} = 200 GeV at STAR
- Brief introduction from the PWG conveners (5’) [Matt Posik]
- Paper proposal (15') [Presentation by Xiaoxuan Chu]
- Open discussions (35')
- Summary from the conveners' panel (5’)
Analysis note: https://drupal.star.bnl.gov/STAR/system/files/dipi0Corr_note_v1.pdf
NOTES
2) Isobar data status: production, QA and centrality
- production: the completion might happen next Feb. Now 25% completed. A few interruptions recently.
- QA: no QA is done for the ongoing production since the production library is exactly the same as Phase-2.
- Centrality: Grigory contacted relevant people who worked on isobar centrality before, and is currently waiting for responses. Will work with production team later to give them access to data that are being produced.
Conclusion: PAC will follow up with Grigory to make sure the centrality classification is done in a timely fashion.
3) Data production/restoration discussion (priority)
i) 2005 Cu+Cu data (cuProductionMinBias and cuProductionHighTower): ~83k MuDst files are requested to be restored by the system. Is there anyone using them?
- Corresponding PicoDst files were/will be restored
Conclusion: it was proposed to halt the MuDst restoration for 2005 Cu+Cu data and remove all the MuDst files from the distributed disk. No objections were raised.
ii) New requests for data restoration
a) LFSUPC: st_upc MuDst files, AuAu_200_producti
b) Cold QCD: st_physics, st_fms, MuDst files, dAu200_production_2016
c) HF: st_physics, PicoDst files, AuAu_200_production_2016, P16ij_SL20c
Conclusion: the LFSUPC and ColdQCD requests are added to the end of the queue as the default, while the HF request is granted higher priority since three analyses at advanced stages are waiting for the data to proceed.
iii) New request for data production
a) Run17 pp 510 GeV st_rp stream to apply the latest space charge corrections
Conclusion: will discuss with the production team to see if this request can be produced on Cori.
4) Analysis meeting: PWG report or analysis highlight
- PWG report: Cold QCD
- Analysis highlight: HF
Conclusion: FCV, CF and LFSUPC decided to have PWG reports, while JetCorr is not decided yet.
5) Followup discussions:
- List of express production on HLT farm to keep. Disk space needs to be freed before Run21 starts.
Conclusion: Dan Cebra has drafted a list of data sets to be kept with specified number of events. See the list here: LIST. Also included in the list is the proposed new priority for BES-II data sets. Conveners will take a look at the proposal and bring the discuss to the PWG if needed.
Next PWGC meeting: Jan. 15th
Happy Holidays!
STAR PWGC meeting
Updated on Fri, 2021-02-05 20:52 by luoxf. Originally created by marr on 2020-11-25 17:31. 2021-01-15 09:30
America/New York
Friday, 15 January 2021
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 14:30 (GMT), duration : 00:00
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 14:30 (GMT), duration : 00:00
1) Proposal of Run17 pp 510 GeV data production after Isobar is finished:
Phase I: st_physics + st_rp concurrently for about 1 month
Phase II: st_physics alone until completed
Phase III: st_rp + st_mtd concurrently until completed
Conclusions: conveners agree with the proposed production strategy for Run17 pp 510 GeV
2) Proton feed-down correction slides
Conclusions: Xiaofeng presented an overview of the drawbacks in the published primordial proton spectra based on UrQMD+GEANT for feed-down correction, and two other analyses using these published spectra. The feed-down correction based on UrQMD+GEANT is different from that based on recently published strange hadron yields (PRC 102 (2020) 34909) both in magnitude and collision energy dependence. A few action items to followup:
- Collect inclusive proton spectra at BES-I energies used in R_cp PRL paper, and compare them to PRC 96 (2017) 44904 and PRC 101 (2020) 24905. This is to understand differences and systematics
- Compare to proton spectra published by other collaborations, e.g. NA49, at relevant energies
- Continue to discuss how to release the primordial proton spectra with feed-down correction based on measured strange hadron yields
3) Data restoration request: priority list
Cold QCD: Run17 pp 510 GeV st_physics, P20ic MuDst, RunList
Conclusions: the Cold QCD PWG will check whether the jet trees produced for st_physics during data production can fulfill analyzers' needs. If so, there is no need to restore the requested MuDst at the moment
4) Discussion: proposal from Dan
- List of express production on HLT farm to keep. Disk space needs to be freed before Run21 starts.
- Revisit BES-II production priority
Conclusions:
- the convener panel agrees with Dan's proposal in terms of what datasets to keep on pwg_tasks space from HLT express production. The list will be forwarded to the TFG to take action.
- the BES-II data production priority (priority list) is modified according to Dan's proposal with some minor adjustments
5) Collaboration meeting, March 1-12, ~9am - 2pm BNL time
6) Upcoming conferences
Phase I: st_physics + st_rp concurrently for about 1 month
Phase II: st_physics alone until completed
Phase III: st_rp + st_mtd concurrently until completed
Conclusions: conveners agree with the proposed production strategy for Run17 pp 510 GeV
2) Proton feed-down correction slides
Conclusions: Xiaofeng presented an overview of the drawbacks in the published primordial proton spectra based on UrQMD+GEANT for feed-down correction, and two other analyses using these published spectra. The feed-down correction based on UrQMD+GEANT is different from that based on recently published strange hadron yields (PRC 102 (2020) 34909) both in magnitude and collision energy dependence. A few action items to followup:
- Collect inclusive proton spectra at BES-I energies used in R_cp PRL paper, and compare them to PRC 96 (2017) 44904 and PRC 101 (2020) 24905. This is to understand differences and systematics
- Compare to proton spectra published by other collaborations, e.g. NA49, at relevant energies
- Continue to discuss how to release the primordial proton spectra with feed-down correction based on measured strange hadron yields
3) Data restoration request: priority list
Cold QCD: Run17 pp 510 GeV st_physics, P20ic MuDst, RunList
Conclusions: the Cold QCD PWG will check whether the jet trees produced for st_physics during data production can fulfill analyzers' needs. If so, there is no need to restore the requested MuDst at the moment
4) Discussion: proposal from Dan
- List of express production on HLT farm to keep. Disk space needs to be freed before Run21 starts.
- Revisit BES-II production priority
Conclusions:
- the convener panel agrees with Dan's proposal in terms of what datasets to keep on pwg_tasks space from HLT express production. The list will be forwarded to the TFG to take action.
- the BES-II data production priority (priority list) is modified according to Dan's proposal with some minor adjustments
5) Collaboration meeting, March 1-12, ~9am - 2pm BNL time
- Mar. 1-5: parallel sessions
- Mar. 8-12: plenary sessions
6) Upcoming conferences
- sQM 2021, May, coming soon
- DIS 2021, April 12-16, abstract due Feb. 1st, online: https://indico.bnl.gov/event/9726/
- CPOD, 2021 March 15-19, abstract due Feb. 15th, online: https://indico.cern.ch/event/985460/
STAR PWGC meeting
Updated on Fri, 2021-01-22 12:28. Originally created by marr on 2020-11-25 17:31. 2021-01-22 09:30
America/New York
Friday, 22 January 2021
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 14:30 (GMT), duration : 00:00
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 14:30 (GMT), duration : 00:00
1) Paper preview: Measurement of Jpsi production within charged jets in p+p collisions at sqrt(s) = 500 GeV with the STAR experiment
- Brief introduction from the PWG conveners (5’) [Yi Yang]
- Paper proposal (15') [Presentation by Qian Yang]
- Open discussions (35')
- Summary from the conveners' panel (5’)
Proposal page: https://www.star.bnl.gov/protected/heavy/tc88qy/web/Jpsi_in_jet_pp/
NOTES
2) Run 10 AuAu200_production, P10ik. Are the MuDst files of the following file streams used? (The number is the missing number of MuDst files for each stream on DD)
st_atomcules: 25057
st_gamma: 15808
st_hlt: 24836
st_ht: 40548
st_mtd: 20438
st_physics: 2018
st_pmdftp: 2969
st_upc: 15866
st_upsilon: 111
st_zerobias: 8341
Conclusions: the st_upc stream will be kept on distributed disk without restoring the missing files, while all other non-st_physics streams will be removed.
STAR PWGC meeting
Updated on Sun, 2021-01-31 21:14. Originally created by marr on 2020-11-25 17:31. 2021-01-29 09:30
America/New York
Friday, 29 January 2021
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 14:30 (GMT), duration : 00:00
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 14:30 (GMT), duration : 00:00
1) Paper preview: Measurement of Elastic Cross Section in Proton--Proton Collisions at $\sqrt{s} = 510$~GeV
- Brief introduction from the PWG conveners (5’) [Nasim]
- Paper proposal (15') [Presentation by Wlodek]
- Open discussions (35')
- Summary from the conveners' panel (5’)
Proposal page: https://drupal.star.bnl.gov/STAR/pwg/lfs-upc/gpc-paper-review-pp-elastic-scattering-510-gev
NOTES
2) Procedure for approving derived plots from published data (PROPOSED PROCEDURE)
Conclusions: the proposed procedure is suggested to be only applied to cases where internal information is used.
3) Upcoming collaboration meeting: please start soliciting contributions for parallel sessions
- Junior's day on March 1st. Please avoid scheduling parallel sessions on this day
- Suggestions for physics highlight talks
- Convener-management meeting on Friday after the collaboration meeting ends
4) Submitted presentation
5) Upcoming conferences
- sQM 2021, May, coming soon
- DIS 2021, April 12-16, abstract due Feb. 1st, online: https://indico.bnl.gov/event/9726/
- CPOD, 2021 March 15-19, abstract due Feb. 15th, online: https://indico.cern.ch/event/985460/
STAR PWGC meeting
Updated on Fri, 2021-02-05 23:15. Originally created by marr on 2020-11-25 17:31. 2021-02-05 09:30
America/New York
Friday, 5 February 2021
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 14:30 (GMT), duration : 00:00
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 14:30 (GMT), duration : 00:00
1) Paper preview: Light nucleus v1 and v2 from 3 GeV Au+Au collisions
- Brief introduction from the PWG conveners (5’) [ShinIchi]
- Paper proposal (15') [Presentation by Xionghong He]
- Open discussions (35')
- Summary from the conveners' panel (5’)
Proposal page: https://drupal.star.bnl.gov/STAR/blog/hexh/light-nucleus-v1-and-v2-3-gev
NOTES
2) Data production and calibration
Isobar
- DAQ -> PicoDst mostly done. Reprocess failed jobs now.
- PicoDst transfer to DD already started. About 15% done.
- pi/K/P embedding will start soon
- plan for non-cme analyzers: suggest to announce to the collaboration once data are restored to distributed disk
Conclusions: will announce to the collaboration when the PicoDst files are transferred to distributed disk. However, before the CME paper is submitted, i) no analyses that could possibly be used to infer CME signals will be shown as preliminary; ii) the convener panel should be informed of any preliminary results based on the Isobar data even if they are not related to CME in any way
MuDst->PicoDst
- Will resume Run14 AuAu production soon
Run17 pp 510 GeV
- Will resume soon.
- Production plan:
-- Phase I: st_physics + st_rp concurrently for about 1 month
-- Phase II: st_physics alone until completed
-- Phase III: st_rp + st_mtd concurrently until completed
BES-II calibration
- TPC alignment remains the bottleneck
- TPC calibration review underway
-- Expected outcome: either conclude with the available calibration or find some solution to improve the calibration, then proceed with the BES-II production. The review focus is on the BES-II dataset
-- Time line: end of March
3) Shall we count the 3M 7.7 GeV events taken in 2020 towards the 100M goal? Do analyzers foresee to use this portion of the data?
Conclusions: suggest to include the 7.7 GeV data taken in 2020 towards the 100M goal. These data can be used once produced.
4) Collaboration meeting: physics highlight talks from PWGs
Conclusions: conveners will follow up on this
No PWGC meeting next week
STAR PWGC meeting
Updated on Wed, 2020-11-25 17:31. Originally created by marr on 2020-11-25 17:31. 2021-02-12 09:30
America/New York
Friday, 12 February 2021
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 14:30 (GMT), duration : 00:00
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 14:30 (GMT), duration : 00:00
STAR PWGC meeting
Updated on Fri, 2020-12-11 15:20. Originally created by marr on 2020-11-25 17:31. 2020-12-11 09:30
America/New York
Friday, 11 December 2020
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 14:30 (GMT), duration : 00:00
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 14:30 (GMT), duration : 00:00
1) Paper preview: Polarized Light-gluon Collisions: tomography of nuclei at ultra-relativistic speed
- Brief introduction from the PWG conveners (5’) [Dan Cebra]
- Paper proposal (15') [Presentation by Daniel Brandenburg]
- Open discussions (35')
- Summary from the conveners' panel (5’)
Proposal page: https://www.star.bnl.gov/protected/lfsupc/jdb/papers/rho/public/
NOTES
2) IS2021 merged abstract: 1 for LFSUPC, and 1 for FCV
Conclusions: the merged abstract from LFSUPC has been approved. FCV conveners will work on the merged abstract soon.
3) Followup discussions:
- List of express production on HLT farm to keep. Disk space needs to be freed before Run21 starts.
- Isobar embedding request
Conclusions:
- Discussion on the datasets to be kept is still ongoing, which hopefully can converge soon.
- The Isobar embedding request put forward by the JetCorr PWG also satisfies the needs for the LFSUPC. Will put this as a high priority and get it produced soon.
Plenary session III
Updated on Sat, 2020-12-12 16:37. Originally created by marr on 2020-11-25 13:24.| Time | Talk | Presenter |
|---|---|---|
| 09:00 | HF PWG analysis highlight: Jpsi RpA with MTD ( 00:20 ) 1 file | Rongrong Ma |
| 09:20 | JetCorr PWG report ( 00:20 ) 1 file | Raghav Elayavalli |
| 09:40 | Cold QCD PWG report ( 00:20 ) 1 file | Maria Zurek |
| 10:00 | FCV PWG report ( 00:20 ) 0 files | ShinIchi Esumi |
| 10:20 | CF PWG report ( 00:20 ) 1 file | Hanna Zbroszczyk |
| 10:40 | LFSUPC PWG report ( 00:20 ) 1 file | Md Nasim |
Plenary session II
Updated on Sat, 2020-12-12 16:35. Originally created by marr on 2020-11-25 13:24.| Time | Talk | Presenter |
|---|---|---|
| 09:00 | Small system event activity ( 00:30 ) 1 file | Tong Liu |
| 09:30 | Potential issue for 200 GeV Au+Au centrality ( 00:30 ) 1 file | Jiangyong Jia |
| 10:00 | Startless T0 for PID in high luminosity pp/pAu data ( 00:30 ) 1 file | Bassam Aboona |
| 10:30 | BES-II analysis status and plans, CPOD 2021 plans ( 00:30 ) 1 file | Xiaofeng Luo |
Plenary session I
Updated on Sat, 2020-12-12 16:34. Originally created by marr on 2020-11-25 13:23.| Time | Talk | Presenter |
|---|---|---|
| 08:55 | Spokesperson welcome ( 00:05 ) 0 files | Helen Caines & Lijuan Ruan |
| 09:00 | Pythia tuning task force report ( 00:15 ) 1 file | Matt Kelsey |
| 09:15 | Tracking efficiency task force report ( 00:15 ) 1 file | Petr Chaloupka |
| 09:30 | Data production and calibration ( 00:30 ) 1 file | Gene Van Buren |
| 10:00 | Embedding status ( 00:30 ) 1 file | Xianglei Zhu |
| 10:30 | Isobar paper status and plans ( 00:30 ) 2 files | Jamie Dunlop |
STAR Analysis Meeting - January 2021
Updated on Fri, 2021-01-08 13:19. Originally created by marr on 2020-11-25 13:16. 2021-01-06 09:00
2021-01-08 11:00
America/New York
from Wednesday, 6 January 2021 to Friday, 8 January 2021
Online
Online
Conference organizing committee information :
Conference duration: 3 days
=======================================Meeting layout
Plenary sessions only