STAR Correlations and Fluctuations PWG

[AYON MUKHERJEE <ayon.mukherjee AT ttk.elte.hu>]

Thank you, Toshihiro, for going through the manuscript diligently and 
for commenting!

I have incorporated your comments and re-uploaded.

Thanks, also, for signing-off on the proceedings!

With regards,
Ayon.

On 12/05/2023 6:57 am, webmaster--- via Star-cf-l wrote:
> Dear star-cf-l AT lists.bnl.gov members,
>
> Toshihiro Nonaka ( tnonaka AT rcf.rhic.bnl.gov ) has commented on a material
> originally submitted by Ayon Mukherjee ( mukherjee AT caesar.elte.hu ) at
> https://drupal.star.bnl.gov/STAR/presentations/Zimanyi-School-2022/Kaon-femtoscopy-L%C3%A9vy-sources-200-GeV-Au-Au-collisions-STAR
>
> Comment:
> Dear Ayon,
>
> I have some minor comments on your very nice proceedings.
>
> With these considered, I sign off.
>
> Best regards,
> Toshihiro
>
> L5:
> - created at RHIC -> at RHIC
> - Preliminary analysis of said data hints  -> Preliminary results hint
>
> L7-8: ... studies at lower center-of-mass energies may... (remove comma)
>
> L66: center-of-mass energy
>
> L74: phase transition
>
> L81: QCD phase diagram
>
> L112: center-of-mass energy per nucleon pair
>
> L118: centrality range
>
> L119: kaon identification with energy loss measured...
>
> L120: distance of closest approach
>
> L127: background events
>
> L130: correlation function
>
> L157: fit range
>
> L187: critical end point
>
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov
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--
Dr. Ayon Mukherjee
Research Fellow
Institute of Physics
Eötvös Loránd Tudományegyetem (ELTE)
Egyetem tér 1-3
H-1053 Budapest
Hungary