STAR Flow, Chirality and Vorticity PWG

[ShinIchi Esumi <esumi.shinichi.gn AT u.tsukuba.ac.jp>]

Dear Kosuke
Thanks for the head up. We appreciate you very much. 
I would like to see some correlated information between 
some variables, for example, multiplicity correlation between 
different detectors or Q-vector correlations or z-vertex 
dependences, or correlation between different information 
for a give track like beta (or de/dx) vs p or Nhit vs eta (or pT)
etc, however since you might also like to see the time variation 
of these correlations, (but it’s in 2D) so you could integrate 
these correlations within a wide time window, that could be 
much coarse or rough compared to all the variables you 
listed here to look at these 1D information in much more 
finer steps, right? Do you also plan to see event averaged 
DCA quantities that we found it’s important for checking 
the TPC ion-feed-back (beam related) with <DCA> per 
event, which has quite a good sensitivity with good accuracy 
in the central events, since there are many tracks.  
Best regards, ShinIchi

> On Sep 23, 2020, at 11:00, kokubo via Star-fcv-l <star-fcv-l AT lists.bnl.gov> 
> wrote:
> 
> Dear conveners and all,
> 
> With the upcoming production for 2018 isobar data, the QA Board will be 
> requiring to do the QA of the isobar production.
> 
> The production will be started soon, I have prepared a list of run by run 
> QA for FCV group.
> The list can be found on the link below.
> https://drupal.star.bnl.gov/STAR/system/files/runbyrun_isobar.pdf
> 
> I would like to request conveners and all the group members  to for their 
> suggestions if any other additional run by run QA need to be included.
> 
> Best regards,
> Kosuke
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