STAR Flow, Chirality and Vorticity PWG

[Cameron Racz <cracz001 AT ucr.edu>]

Hi Subhash,

I am currently analyzing the P23id/SL23d versions of all of the following 
datasets since they are not all updated in P23ie/SL23e versions and I would 
like to stay consistent across energies. I would appreciate if we could keep 
the 23d versions, at least until this analysis is complete.

    • production_4p59GeV_fixedTarget_2019
    • production_5p75GeV_fixedTarget_2020
    • production_7.3GeV_fixedTarget_2019
    • production_7p3GeV_fixedTarget_2020
    • production_9p8GeV_fixedTarget_2020

Cameron Racz
Ph.D. Candidate 
Heavy-ion Physics Group
University of California, Riverside






> On Jan 28, 2024, at 11:38 PM, subhash via Star-fcv-l 
> <star-fcv-l AT lists.bnl.gov> wrote:
> 
> Dear All,
> 
> We have discussed during the PWGC meeting that we are identifying datasets 
> that can be deleted from the DD.
> 
> MuDsts on DDs: 
> https://www.star.bnl.gov/public/comp/prod/localdata/ProdDDstreams.html
> Please let us know asap if there is any active analysis (or papers in GPC) 
> using any MuDsts (especially before 2014 productions).
> 
> PicoDsts on DD: 
> https://www.star.bnl.gov/public/comp/prod/localdata/ProdDDstreams_pico.html
> There are PicoDst productions with multiple libraries. The Picodsts with 
> latest libraries will be kept but with the old libraries will likely be 
> removed depending on your need/feedback. So let us know.
> 
> 
> Thanks and regards,
> FCV conveners
> 
> -- 
> --------------------------
> Subhash Singha
> Institute of Modern Physics
> Chinese Academy of Sciences
> Office: +86 18693107172
> Skype: subhash.singha1
> https://urldefense.com/v3/__http://about.me/ssingha__;!!P4SdNyxKAPE!D59kCQed_wJCk0-VMEMgDIlf4CDxXe1J-owAr7i8PIYFETHFD-aAisD7kvCw3iGcWqPQTejCFryYCPsYPtoobYg5IQ$
>  
> --------------------------
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