STAR Flow, Chirality and Vorticity PWG

[subhash <subhash AT rcf.rhic.bnl.gov>]

Dear All,

You may have seen email from Rongrong (see below) that we are collecting 
inputs for data production priorities keeping QM'23 in mind. Please let 
us know if you or your group are involved/interested in analysis for O+O 
or d+Au systems targeting for QM? It will help us setting up priority of 
production for these datasets.

Thanks and regards,
Subhash
for FCV conveners

ps:Here is Rongrong's email:

4) Data production priority (PRIORITY LIST)
https://drupal.star.bnl.gov/STAR/pwg/common/production-priorties
Run21: O+O vs. d+Au
Production time: 2 weeks each
Calibration time: d+Au - 4 weeks; O+O - a few months
Run22: st_physics, st_mtd, st_fwd, st_W, st_upc, st_zerobias
Conclusions:
- One suggestion: (Run20+21) 26.5 FXT (7.2) > 3.85 FXT I (3.0) > 44.5 
FXT (9.2) > 70 FXT (11.5) > 100 FXT (13.7) > 200 GeV d+Au  > 200 GeV O+O 
>? 17.3 COL  > 3.85 FXT II (3.0). Will continue the discussion next week.
- PWGs are asked to poll the interests of analyzing O+O data for QM
- Suggested Run 22 priority: st_upc > st_zerobias > st_W > st_physics > 
st_fwd > st_mtd
-- ColdQCD PWG will determine a list of runs for EMC calibration, which 
could be produced before physics production
-- it should be very fast to produce st_upc and st_zerobias streams
-- need to discuss with S&C team whether it is efficient to produce 
st_zerobias stream standalone and couple it with other data streams

--
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Subhash Singha
Institute of Modern Physics
Chinese Academy of Sciences
Office: +86 18693107172
Skype: subhash.singha1
http://about.me/ssingha
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