STAR Correlations and Fluctuations PWG

[Grigory Nigmatkulov <nigmatkulov AT gmail.com>]

Dear Takafumi, Hanna and Xiaofeng,

Thank you very much for your nice comments. Please find the updated version attached:

https://drupal.star.bnl.gov/STAR/system/files/Nigmatkulov_Nucleus2022_v4.pdf

Please find responses below.

>s3: Resolution of the bottom table is not so good. If possible, please replace it with better one.

I tried my best.

>s8: In 1st bullet, “at kinetic freeze-out” This would be true only when using hadrons (which is the most of cases though…)

I agree and removed "at kinetic freeze-out".

>s9: In title, I would remove “in Au+Au Collisions” or replace it with “Heavy-Ion Collisions” since you show results from ALICE and other experiments and mention "2.76 TeV”

Done

>s10: 

>- Left-bottom, larger than that those for -> larger than those for

>- Right-top, since you give a talk on behalf of STAR, please remove STAR collaborator name (and conference name)

Done

>s11: Same comment on removing STAR collaborator name

Done

>s12: Same comment on removing STAR collaborator name except “Anna Kraeva’s talk”

Done

>s13: you may want to mention how the collectivity is studied/visible via Femtoscopy, e.g. kT dependence of radius

Text added.

>Still incorrect. Should be: q_{inv} = \sqrt{(p_1 - p_2)^2 - (E_1 - E_2)^2} 

>Check here for a reference: Phys.Rev.C83:064905,2011

The used equation is correct and is identical to the one from the paper.

Best regards,

Grigory