STAR Flow, Chirality and Vorticity PWG

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

Dear Ankita,
  As per the last CME focus group meeting and a follow-up discussion 
among the conveners we conclude that we are not ready to show any 
physics plot for this poster due to limited vetting. We can show 
performance plots. Our suggestion for your poster is the following:

1. Only can show Fig.2, 4,5, 8, 11 and 12, we're not ready to show the 
rest.

2. You're welcome to show results from: https://arxiv.org/abs/2210.14027
For example, you can replace your Fig.9 and 10 with the published Fig.4 
from 2210.14027

3. Motivate your analysis with the published paper, the theory paper by 
Wang et. al. and introduce your method using ESE that has the promise to 
reduce background.

4. We cannot conclude: "We observe positive intercepts for 20-50% 
collision centralities using ESE"
We can say "ESE approach looks promising to reduce background, work in 
progress"

Can you please modify your poster accordingly. We will send more 
comments on the texts.

Best,
Prithwish




On 2023-02-04 12:30, webmaster--- via Star-fcv-l wrote:
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Ankita Nain (nainankita55555 AT gmail.com) has submitted a material for a
> review, please have a look:
> https://drupal.star.bnl.gov/STAR/node/62448
>
> Deadline: 2022-11-10
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov
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