STAR Flow, Chirality and Vorticity PWG

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

Dear Prithwish and all isobar PAs
I sign off your nice abstract as it is. If I’m allowed to add a few words... 
I would suggest to add that several different CME observables have been 
tested, where the most of delta_gamma related signals are below one, which 
is close to the multiplicity different, while the R2 observable is much 
closer 
to one, maybe because of the definition by construction, though. Further 
differential studies are being pursued as the post blinding analysis… as I 
would hope to have some new insights before the QM. 
Best regards, ShinIchi

> On Nov 29, 2021, at 0:30, webmaster--- via Star-fcv-l 
> <star-fcv-l AT lists.bnl.gov> wrote:
> 
> Dear star-fcv-l AT lists.bnl.gov members,
> 
> Prithwish Tribedy (ptribedy AT bnl.gov) has submitted a material for a review, 
>  
> please have a look:
> https://drupal.star.bnl.gov/STAR/node/57412
> 
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