FWD Software
Updated on Fri, 2024-05-17 09:39. Originally created by jdb on 2024-05-17 09:39. 2024-06-21 11:00
America/New York
Friday, 21 June 2024
https://osu.zoom.us/j/92668696344?pwd=UVpzV2FmeU8ycGtaUzVtQ3FTNjJzdz09, at 15:00 (GMT), duration : 00:00
https://osu.zoom.us/j/92668696344?pwd=UVpzV2FmeU8ycGtaUzVtQ3FTNjJzdz09, at 15:00 (GMT), duration : 00:00
| Time | Talk | Presenter |
|---|---|---|
| 10:00 | FWD software updates ( 00:20 ) 0 files | Daniel |
| 10:20 | FWD Software Updates ( 00:20 ) 1 file | Daniel |
FWD Software
Updated on Fri, 2024-05-17 09:39. Originally created by jdb on 2024-05-17 09:39. 2024-06-14 11:00
America/New York
Friday, 14 June 2024
https://osu.zoom.us/j/92668696344?pwd=UVpzV2FmeU8ycGtaUzVtQ3FTNjJzdz09, at 15:00 (GMT), duration : 00:00
https://osu.zoom.us/j/92668696344?pwd=UVpzV2FmeU8ycGtaUzVtQ3FTNjJzdz09, at 15:00 (GMT), duration : 00:00
FWD Software
Updated on Fri, 2024-05-17 09:39. Originally created by jdb on 2024-05-17 09:39. 2024-06-07 11:00
America/New York
Friday, 7 June 2024
https://osu.zoom.us/j/92668696344?pwd=UVpzV2FmeU8ycGtaUzVtQ3FTNjJzdz09, at 15:00 (GMT), duration : 00:00
https://osu.zoom.us/j/92668696344?pwd=UVpzV2FmeU8ycGtaUzVtQ3FTNjJzdz09, at 15:00 (GMT), duration : 00:00
| Time | Talk | Presenter |
|---|---|---|
| 12:00 | First look: J/psi in data picoDsts ( 00:15 ) 1 file | Isaac Mooney (Yale / BNL) |
FWD Software
Updated on Fri, 2024-05-17 09:39. Originally created by jdb on 2024-05-17 09:39. 2024-05-31 11:00
America/New York
Friday, 31 May 2024
https://osu.zoom.us/j/92668696344?pwd=UVpzV2FmeU8ycGtaUzVtQ3FTNjJzdz09, at 15:00 (GMT), duration : 00:00
https://osu.zoom.us/j/92668696344?pwd=UVpzV2FmeU8ycGtaUzVtQ3FTNjJzdz09, at 15:00 (GMT), duration : 00:00
FWD Software
Updated on Fri, 2024-05-17 09:39. Originally created by jdb on 2024-05-17 09:39. 2024-05-24 11:00
America/New York
Friday, 24 May 2024
https://osu.zoom.us/j/92668696344?pwd=UVpzV2FmeU8ycGtaUzVtQ3FTNjJzdz09, at 15:00 (GMT), duration : 00:00
https://osu.zoom.us/j/92668696344?pwd=UVpzV2FmeU8ycGtaUzVtQ3FTNjJzdz09, at 15:00 (GMT), duration : 00:00
FWD Software
Updated on Fri, 2024-05-17 09:36. Originally created by jdb on 2024-05-17 09:36. 2024-05-17 11:00
America/New York
Friday, 17 May 2024
https://osu.zoom.us/j/92668696344?pwd=UVpzV2FmeU8ycGtaUzVtQ3FTNjJzdz09, at 15:00 (GMT), duration : 00:00
https://osu.zoom.us/j/92668696344?pwd=UVpzV2FmeU8ycGtaUzVtQ3FTNjJzdz09, at 15:00 (GMT), duration : 00:00
The base QA at 17.3GeV of triton
Updated on Thu, 2024-05-16 21:55. Originally created by fangyi on 2024-05-16 21:55.
The base QA at 11.5GeV of hypertriton
Updated on Thu, 2024-05-16 21:54. Originally created by fangyi on 2024-05-16 21:51.CPOD_PremilinaryRequest
Updated on Thu, 2024-05-16 17:30. Originally created by iponce on 2024-05-16 17:19.
Au+Au 3.2 GeV H4L production prelimianry request
Updated on Wed, 2024-05-29 15:18. Originally created by jiyj on 2024-05-16 16:09.This page is preliminary request for 3.2 GeV H4L pt spectra, dN/dy, mean pT in 0-10%, 10-40% and 0-40%
Baryon-Junction-STAR-paper-05162024
Updated on Thu, 2024-05-16 13:38. Originally created by ctsang on 2024-05-16 13:38.
He4L production at 3.2 and 3.5 GeV Preliminary request
Updated on Tue, 2024-05-21 10:13. Originally created by clhu on 2024-05-16 12:33.1. 3.2 GeV H4L preliminary reqeust from Yuanjing Ji:
Preliminary Request of Strangeness Production at 3.2 - 4.5 GeV For CPOD and SQM2024
Updated on Sat, 2024-05-25 04:57. Originally created by lhc on 2024-05-16 10:34.This web page list the preliminray figure for stangeness (Ld and Xi) production analysis at 3.2 -4.5 GeV.
The preliminary request slides in this web link:
STAR Highlights
Updated on Thu, 2024-05-16 08:44. Originally created by rksooraj on 2024-05-16 08:44.Reference
Speaker : Sooraj Radhakrishnan
Talk time : 11:30, Duration : 00:30
D0-pi femtoscopy, Run 2016 & Run 2014 comparison (SQM)
Updated on Thu, 2024-05-16 08:18. Originally created by priyankawut on 2024-05-16 08:10.Inclusive D0-jets Run14 Au+Au - raw data proposal
Updated on Thu, 2024-05-16 03:06. Originally created by lomicond on 2024-05-16 03:06.
STAR PWGC meeting
Updated on Thu, 2024-07-18 08:09 by rksooraj. Originally created by marr on 2024-05-15 20:58. 2024-07-19 10:00
America/New York
Friday, 19 July 2024
https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 14:00 (GMT), duration : 00:00
https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 14:00 (GMT), duration : 00:00
1) Paper preview: Measurements of Proton−Proton, Proton−Λ and Proton−Ξ- Correlation Functions in sqrt{sNN} = 3 GeV Au+Au Collisions at RHIC
- Brief introduction from the PWG conveners (5’) [Hanna Zbroszczyk]
- Paper proposal (15') [Presentation by Chuan Fu]
- Brief introduction from the PWG conveners (5’) [Hanna Zbroszczyk]
- Open discussions (35')
- Summary from the conveners' panel (5’)
2) STAR Online Analysis Meeting
- Tentatively September 9 - 11, 2024, focused mainly on HP
- Will keep to morning sessions
2) STAR Online Analysis Meeting
- Tentatively September 9 - 11, 2024, focused mainly on HP
- Will keep to morning sessions
STAR PWGC meeting
Updated on Mon, 2024-07-15 12:15 by rksooraj. Originally created by marr on 2024-05-15 20:57. 2024-07-12 10:00
America/New York
Friday, 12 July 2024
https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 14:00 (GMT), duration : 00:00
https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 14:00 (GMT), duration : 00:00
1) Paper preview: Observation of Centrality-Dependent Difference in Directed flow between Charged Kaons and K* Resonances in Au+Au collisions at √sNN = 19.6 and 27 GeV
- Brief introduction from the PWG conveners (5’) [Zhenyu Chen]
- Paper proposal (15') [Presentation by Md Nasim]
- Brief introduction from the PWG conveners (5’) [Zhenyu Chen]
- Open discussions (35')
- Summary from the conveners' panel (5’)
2) Update from tracking efficiency uncertainty task force
- Presentation by Petr Chaloupka
- Plans
3) Quoting systematic uncertainties in STAR results and measurements
- Some results/groups use differences between variations divided by sqrt(12) as the systematic uncertainty while others quote just the difference
- Dividing by sqrt(12) relies on some assumptions - that the variation is uniformly distributed and that the change of cuts capture the range of variations. For the cases that divide the difference by sqrt(12) it should be shown that the assumptions are satisfied
2) Update from tracking efficiency uncertainty task force
- Presentation by Petr Chaloupka
- Plans
3) Quoting systematic uncertainties in STAR results and measurements
- Some results/groups use differences between variations divided by sqrt(12) as the systematic uncertainty while others quote just the difference
- Dividing by sqrt(12) relies on some assumptions - that the variation is uniformly distributed and that the change of cuts capture the range of variations. For the cases that divide the difference by sqrt(12) it should be shown that the assumptions are satisfied
STAR PWGC meeting
Updated on Fri, 2024-07-05 08:51 by rksooraj. Originally created by marr on 2024-05-15 20:57. 2024-07-05 10:00
America/New York
Friday, 5 July 2024
https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 14:00 (GMT), duration : 00:00
https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 14:00 (GMT), duration : 00:00
1) Paper preview: Inclusive Hadron Yield Analysis in Small and Mid-sized Collision Systems at sqrt{s_NN} = 200 GeV at STAR
- Brief introduction from the PWG conveners (5’) [] - Paper proposal (15') [Presentation by Tong Liu, Maowu Nie]
- Open discussions (35')
- Summary from the conveners' panel (5’)
2) Quoting systematic uncertainties in STAR results and measurements
- Some results/groups use differences between variations divided by sqrt(12) as the systematic uncertainty while others quote just the difference
- Dividing by sqrt(12) relies on some assumptions - that the variation is uniformly distributed and that the change of cuts capture the range of variations. For the cases that divide the difference by sqrt(12) it should be shown that the assumptions are satisfied
2) Quoting systematic uncertainties in STAR results and measurements
- Some results/groups use differences between variations divided by sqrt(12) as the systematic uncertainty while others quote just the difference
- Dividing by sqrt(12) relies on some assumptions - that the variation is uniformly distributed and that the change of cuts capture the range of variations. For the cases that divide the difference by sqrt(12) it should be shown that the assumptions are satisfied
STAR PWGC meeting
Updated on Thu, 2024-06-27 12:53 by rksooraj. Originally created by marr on 2024-05-15 20:57. 2024-06-28 10:00
America/New York
Friday, 28 June 2024
https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 14:00 (GMT), duration : 00:00
https://lbnl.zoom.us/j/99981267001?pwd=Q05nbjc3ZlgvR21TTzFpK2Jod2pJdz09, at 14:00 (GMT), duration : 00:00
1) Paper preview: Probing Late-Stage Hadronic Interactions at High Baryon Density via K*0 Production in the RHIC Beam Energy Scan Program
- Brief introduction from the PWG conveners (5’) [Yue-Hang Leung]
- Open discussions (35')
- Summary from the conveners' panel (5’)
2) FXT TPC alignment and data reproduction
- Track breaking at central membrane found to be from TPC alignment issues Presentation from Yuri
- Timeline expected for being ready for reproduction - end of August
2) FXT TPC alignment and data reproduction
- Track breaking at central membrane found to be from TPC alignment issues Presentation from Yuri
- Timeline expected for being ready for reproduction - end of August