STAR Flow, Chirality and Vorticity PWG

[Chunjian Zhang <czhang.phys AT gmail.com>]

Hi Subhash, 

I am using the picoDst and muDst: 

picoDst: SL21c for AuAu200_production; SL19c for AuAu200_production_2011; SL22a for UU_production_2012.

muDst: AuAu_producitons on year 2010 and 2011; UU_produciton_2012

I would appreciate it if we keep SL18c, SL19c, SL21c, SL22a. 

Thanks,

Chunjian 

On Mon, Jan 29, 2024 at 12:38 AM 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
http://about.me/ssingha
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