D_TT vs z in pp collision in run 2015 update
Updated on Wed, 2021-09-29 09:53. Originally created by yxu on 2021-09-29 09:48.Run22 triggers
Updated on Wed, 2021-09-29 07:07. Originally created by akio on 2021-09-29 07:07.Reference
Speaker : Akio
Talk time : 12:20, Duration : 00:20
https://www.star.bnl.gov/protected/spin/akio/fcs/run22trg.html
TPC readout for FCS triggers
Updated on Wed, 2021-09-29 07:05. Originally created by akio on 2021-09-29 07:05.longitudinal spin transfer $D_{LL}$ vs z of $\Lambda$ hyperon for pp200long2_2015
Updated on Thu, 2021-09-30 08:17. Originally created by yiyu on 2021-09-29 03:40.This page presents the preliminary results on the longitudinal spin transfer DLL vs z of \Lambda hyperon for 200 GeV p-p collisions of run 15 with the same run list used in the DLL vs pt pr
Preliminary for DNP2021
Updated on Fri, 2021-10-08 02:52. Originally created by dneff on 2021-09-29 01:41.
Discussions on comparison, PID vn ratios and preliminary request for the upcoming DNP conference
Updated on Thu, 2021-10-07 09:03. Originally created by chunjian on 2021-09-28 22:10.FCV meeting 09/29
π0+jet Δφ decorrelations in p+p collisions: Rutgers Collab. meeting 16Sep2021
Updated on Tue, 2021-09-28 21:19. Originally created by nihar on 2021-09-28 21:19.
AOB
Updated on Tue, 2021-09-28 17:46. Originally created by dongx on 2021-09-28 17:46.Daves talk on VSII
Updated on Tue, 2021-09-28 14:54. Originally created by lisa on 2021-09-28 14:54.Here is Dave's abstract. VSII is super-awesome etc.
Reference
Speaker : Dave Kieda ( Utah )
Talk time : 09:00, Duration : 00:20
Intensity Interferometry of single non-rapid-rotator stars
Updated on Tue, 2021-09-28 14:52. Originally created by lisa on 2021-09-28 14:52.| Time | Talk | Presenter |
|---|---|---|
| 09:00 | Daves talk on VSII ( 00:20 ) 0 files | Dave Kieda (Utah) |
Test conference
Updated on Thu, 2021-09-30 12:12. Originally created by lisa on 2021-09-28 14:51. 2022-04-25 14:00
2022-04-27 14:00
America/New York
from Monday, 25 April 2022 to Wednesday, 27 April 2022
Ohio State
Ohio State
Conference organizing committee information : Me, myself, and I.
Conference duration: 3 days
I am just doing a test here. There is not a real conference
»
Calibration Status (14.5 GeV and FXT Run19-20 Datasets)
Updated on Tue, 2021-09-28 12:54. Originally created by dongx on 2021-09-28 12:54.Computing Resource Requests Run23-25 In View of TPC Rate Increase
Updated on Wed, 2021-09-29 10:36 by jml. Originally created by dongx on 2021-09-28 12:52.Reference
Speaker : Jeff Landgraf
Talk time : 12:00, Duration : 00:15
STAR PWGC meeting
Updated on Sat, 2022-03-19 19:01. Originally created by marr on 2021-09-28 10:15. 2022-03-18 09:30
America/New York
Friday, 18 March 2022
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 13:30 (GMT), duration : 00:00
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 13:30 (GMT), duration : 00:00
1) Paper preview: Measurements of charged particle multiplicity dependence of higher-order net-proton cumulants in p+p collisions at √s = 200 GeV from RHIC
- Brief introduction from the PWG conveners (5’) [Hanna Zbroszczyk]
- Paper proposal (15') [Presentation by Risa Nishitani]
- Open discussions (35')
- Summary from the conveners' panel (5’)
PA: Risa Nishitani, Nu Xu, Xiaofeng Luo, Bedanga Mohanty, Toshihiro Nonaka, ShinIchi Esumi, Ashish Pandav, Ho-San Ko, Yu Zhang
Target journal: PRL
NOTES
Target journal: PRL
NOTES
2) Production and embedding status
- Production
- MuDst->PicoDst conversion:
- Run 12 pp st_physics - done, st_zerobias will be produced after QM
- Run 18 Isobar st_hf - done
- DAQ->MuDst->PicoDst production for Run19 200 GeV Au+Au
- Will start soon, if not already
- first pass to use the AuAu vertex finder; users will analyze the data to see if a second pass for UPC events is needed
- PicoDst chain option: PicoVtxDefault PicoCovMtxWrite
- MuDst->PicoDst conversion:
3) StRefMultCorr definition for 19.6 GeV is now ready in DEV. Trigger inefficiency correction for isobar is also updated.
4) New StRefMultCorr maintainer
Conclusions: will follow up on this
5) PWG needs for FCS trigger in Au+Au running (Raghav)
- What triggers need to be prepared, what other running conditions of the detectors are needed, etc.
Conclusions: PWGs should send inputs, which could be no FCS triggers needed, to Raghav over the weekend
AOB:
- For some institutions, a large fraction of their disk quote on RCF is not used, while for some other institutions disk space is critically needed. Will look into if it is possible to utilize those unused disk space.
- No PWGC meeting for the next three weeks due to pre-QM meeting and QM conference
- Path on DEV: /afs/rhic.bnl.gov/star/packages/DEV/StRoot/StRefMultCorr
- Example macro: /star/u/gnigmat/soft/u/refMultCorr/checkStRefMultCorr.C
- Bad run and pileup rejection need to be done explicitly by analyzers by calling functions in StRefMultCorr
4) New StRefMultCorr maintainer
Conclusions: will follow up on this
5) PWG needs for FCS trigger in Au+Au running (Raghav)
- What triggers need to be prepared, what other running conditions of the detectors are needed, etc.
- A short presentation during forward upgrade meeting on Tuesday March 22nd at 8:30 am
Conclusions: PWGs should send inputs, which could be no FCS triggers needed, to Raghav over the weekend
AOB:
- For some institutions, a large fraction of their disk quote on RCF is not used, while for some other institutions disk space is critically needed. Will look into if it is possible to utilize those unused disk space.
- No PWGC meeting for the next three weeks due to pre-QM meeting and QM conference
STAR PWGC meeting
Updated on Tue, 2021-09-28 10:15. Originally created by marr on 2021-09-28 10:15. 2022-03-25 09:30
America/New York
Friday, 25 March 2022
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 13:30 (GMT), duration : 00:00
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 13:30 (GMT), duration : 00:00
STAR PWGC meeting
Updated on Tue, 2021-09-28 10:15. Originally created by marr on 2021-09-28 10:15. 2022-04-01 09:30
America/New York
Friday, 1 April 2022
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 13:30 (GMT), duration : 00:00
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 13:30 (GMT), duration : 00:00
STAR PWGC meeting
Updated on Tue, 2021-09-28 10:15. Originally created by marr on 2021-09-28 10:15. 2022-04-08 09:30
America/New York
Friday, 8 April 2022
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 13:30 (GMT), duration : 00:00
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 13:30 (GMT), duration : 00:00
STAR PWGC meeting
Updated on Fri, 2022-04-15 15:23. Originally created by marr on 2021-09-28 10:15. 2022-04-15 09:30
America/New York
Friday, 15 April 2022
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 13:30 (GMT), duration : 00:00
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 13:30 (GMT), duration : 00:00
1) Possible merging of JetCorr and HF PWGs
Conclusions: conveners are supportive of this proposal. The next step is to bring this up for discussion in JetCorr and HF PWGs, and seek feedback.
2) Data production news
3) Discussion on forward detector triggering in Au+Au
- A followup meeting was proposed by the forward upgrade group on Apr. 26th 8:30am
Conclusions: conveners will bring this up for discussion in PWG meetings next week, and provide feedback. Such a discussion is also needed for this year's BUR, where we need to outline a concrete plan of how to run STAR in 2023-25.
4)Work on BUR highlight section
Conclusions: conveners are supportive of this proposal. The next step is to bring this up for discussion in JetCorr and HF PWGs, and seek feedback.
2) Data production news
- Daq production
-
- Run18 st_mtd, st_upc chains are ready to start
- Run19 & 20 FXT datasets completed. Issue with eTOF. Need a reproduction of MuDst->PicoDst for Run20 FXT
- Run19 AuAu200 done
- MuDst->PicoDst conversion
- Run17 pp500_production, paused due to NFS storage limitation, resume soon
- Run18 isobar st_hf completed
- Calibrations
- Run21 Large calibration production for AuAu7.7 collisions has started
- Run22 pp510
- TPC space charge initial calibration, another iteration has begun
3) Discussion on forward detector triggering in Au+Au
- A followup meeting was proposed by the forward upgrade group on Apr. 26th 8:30am
Conclusions: conveners will bring this up for discussion in PWG meetings next week, and provide feedback. Such a discussion is also needed for this year's BUR, where we need to outline a concrete plan of how to run STAR in 2023-25.
4)Work on BUR highlight section
STAR PWGC meeting
Updated on Fri, 2022-04-22 15:06. Originally created by marr on 2021-09-28 10:15. 2022-04-22 09:30
America/New York
Friday, 22 April 2022
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 13:30 (GMT), duration : 00:00
https://bnl.zoomgov.com/j/1619294511?pwd=TkRhZzFjOWZSQnpvUVdGUGFVMmlHdz09, at 13:30 (GMT), duration : 00:00
1) Possible merging of JetCorr and HF PWGs
Conclusions: generally positive feedback from PWG members so far. Conveners are trying to gather more comments from active members who were not able to join this week's PWG meetings. If no strong objections raised, we will proceed with the merging in the near future.
2) Discussion on forward detector triggering in Au+Au
Conclusions: most of PWGs are fine with reading out forward detectors without triggering on them in Au+Au running. Couple of ideas on triggering were raised, and conveners will follow up with the proponents.
3) Embedding request for Run19 14.6 GeV (intended for sQM)
4) Collect preliminary figures (ARXIV)
Conclusions: it turned out that it is quite difficult, if not impossible, to upgrade Drupal for STAR given the large volume of contents accumulated in the past 20+ years. Therefore, a central repository for preliminary figures on Drupal is unlikely. We will continue the following practice: i) for any new preliminary results, PA should create a Drupal blog page to host the preliminary figures (in pdf format) and preliminary request slides; ii) conveners collect links to these Drupal pages and put them in a central place (ARXIV)
Conclusions: generally positive feedback from PWG members so far. Conveners are trying to gather more comments from active members who were not able to join this week's PWG meetings. If no strong objections raised, we will proceed with the merging in the near future.
2) Discussion on forward detector triggering in Au+Au
Conclusions: most of PWGs are fine with reading out forward detectors without triggering on them in Au+Au running. Couple of ideas on triggering were raised, and conveners will follow up with the proponents.
3) Embedding request for Run19 14.6 GeV (intended for sQM)
- 1 embedding request each for K+, K-, pi+, and pi-
- run 19 Au+Au BESII
- 14.5 GeV (P21ic, production_14p5GeV_2019)
- Minbias Triggers: 650000
- -70cm < Vz < 70cm and Vr < 2cm
- 0-80% Centrality
- 5% refmult particles embedded in each event
- Uniform in Rapidity: [-1.5,1.5]
- Uniform in pT: [0.0,5.0]
- Uniform in phi: [0,2π]
- 1.5M Events
4) Collect preliminary figures (ARXIV)
Conclusions: it turned out that it is quite difficult, if not impossible, to upgrade Drupal for STAR given the large volume of contents accumulated in the past 20+ years. Therefore, a central repository for preliminary figures on Drupal is unlikely. We will continue the following practice: i) for any new preliminary results, PA should create a Drupal blog page to host the preliminary figures (in pdf format) and preliminary request slides; ii) conveners collect links to these Drupal pages and put them in a central place (ARXIV)