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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Maria Stefaniak for Initial Stages 2021 submitted for review

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: ShinIchi Esumi <esumi.shinichi.gn AT u.tsukuba.ac.jp>
  • To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Maria Stefaniak for Initial Stages 2021 submitted for review
  • Date: Wed, 6 Jan 2021 03:51:28 +0900

Dear Maria
Thank you for the nice talk, I would like you to make sure they are consistent to 
what was shown by Peter/Arkadij/Grigory for the previous conference, where they 
have decided to limit in the pT range for the PIDed v2/v3 at that time especially 
for Kaon, because of the possible contaminations, we did not hear any follow-up 
presentation in the PWG afterwards… 
Best regards, ShinIchi

On Jan 5, 2021, at 17:10, Maria Stefaniak via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:

Dear Jiangyong,

Thank you for comments. I applied your suggestions:

regards,
Maria

Wiadomość napisana przez Jiangyong Jia via Star-fcv-l <star-fcv-l AT lists.bnl.gov> w dniu 03.01.2021, o godz. 01:29:

Dear Maria,

A few comments on your nice set of slides.
1) Please add slide number
2) slide2, it would be good to give a short outline, maybe just mention you will present flow decorrelation, PID flow and high pT flow.
3) slide7, remove "development". Also this slide is super busy, you might want to reduce the amount of text and number of figuress
For example, you probably do not need to give the details of the 2PC just mention the gap is enough.
4) slide8, "Significant as a reference for the theoretical studies...". I am confused by this wording, can you be more clear?
5) slide 10 is quote busy,  the the v11 plots on the right,  you probably just need one panel for each. That will simplify the slide.

Jiangyong


On 12/30/20 11:05 AM, webmaster--- via Star-fcv-l wrote:
Dear star-fcv-l AT lists.bnl.gov members,

Maria Stefaniak (mzstefaniak AT gmail.com) has submitted a material for a  
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/53162

---
If you have any problems with the review process, please contact  
webmaster AT www.star.bnl.gov
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Best regards,

MSc Eng. Maria Stefaniak

*********************************************************************************

   Nuclear Physics Division, Warsaw University of Technology
               Theory Group, Subatech Nantes
                      STAR Junior Representative

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