STAR Flow, Chirality and Vorticity PWG

[Prithwish Tribedy <ptribedy AT rcf.rhic.bnl.gov>]

Hello ShinIchi,
  It's great to see contributions supporting the production request.
Here is a small contribution from Nicole and me:

https://drupal.star.bnl.gov/STAR/system/files/run19_200gev_pwgc_production_request_photonuclear.pdf

Best,
Prithwish


On 2021-04-15 07:33, ShinIchi Esumi via Star-fcv-l wrote:
> Dear Maowu
> Thanks for the updates, I wanted to see your fast production analysis
> with isobar data (blue in your right 3rd panel) overlaid. Anyway, they 
> do
> seem to agree at this same centrality in different collision systems, 
> though.
> Best regards, ShinIchi
>
> > On Apr 15, 2021, at 20:16, Maowu Nie <nie AT rcf.rhic.bnl.gov> wrote:
> >
> > Dear ShinIchi,
> >
> > Thanks for the reply.
> > r2 results in Gaoguo's page 13 cannot directly compared with Au+Au 
> > results, since it still has large non-flow contribution for isobar.
> > The eta_ref dependence is in our to-do list with full isobar dataset.
> >
> > I quote one plot of the comparison in Gaoguo's Collaboration Meeting 
> > slides.(https://drupal.star.bnl.gov/STAR/system/files/collaboration_meeting_20210303_GaoguoYan.pdf)
> >
> > You can see a clear offset in Au+Au data, which makes it hard to 
> > compare. This is also another big reason we need run19 Au+Au 200GeV 
> > data.
> > To study the system size dependence of flow decorrelation needs 
> > precise measurements for both systems.
> >
> > The above information are included in the slides with the same link:
> > https://drupal.star.bnl.gov/STAR/system/files/request_run19AuAu200GeV.pdf
> >
> > Hope it helps.
> >
> > Regards,
> > Maowu
> >
> >
> > 在 2021-04-15 18:34，ShinIchi Esumi via Star-fcv-l 写道：
> > > Dear Maowu, Thank you very much.
> > > Please overlay your two plots in your first page with the plots at
> > > shown yesterday
> > > by Gaoguo in his page 13 or show them by side-by-side.
> > > Best regards, ShinIchi
> > > > On Apr 15, 2021, at 17:35, Maowu Nie <nie AT rcf.rhic.bnl.gov> wrote:
> > > > Dear ShinIchi, Prithwish, Jiangyong and FCV enthusiasts,
> > > > As we already discussed yesterday, we would like to request high 
> > > > priority of run19 Au+Au@200GeV data production.
> > > > You can find the request slides below:
> > > > https://drupal.star.bnl.gov/STAR/system/files/request_run19AuAu200GeV.pdf
> > > > Inputs from other related physics interests are also welcome.
> > > > Regards,
> > > > Maowu
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>
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