STAR Flow, Chirality and Vorticity PWG

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Dear star-fcv-l AT lists.bnl.gov members,

Prithwish Tribedy ( ptribedy AT bnl.gov ) has commented on a material originally 
 
submitted by Zhiwan Xu ( zhiwanxu AT physics.ucla.edu ) at
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2023/Search-Chiral-Magnetic-and-Vortical-Effects-Using-Event-Shape-Vari-0

Comment:
Nice slides, I approve with the following comments:

Slide#16:

"ESS and ESE observables have uncertainties too large to conclude at 7.7, 27  
and 200 GeV"
-->
"ESS and ESE results have uncertainties too large to conclude at 7.7, 27 and  
200 GeV"

"The data interpretation requires further assessment of the new ESS  
methodology"
-->
"The data interpretation requires further assessment of the new event-shape  
methodologies"

Make the following line as a sub-bullet of "The data interpretation...."
"In using \Psi_2, low....."


Slide#15:

"CVE measurements of Λ-p Δγ correlation using \Psi_1"
-->
"CVE measurements of Λ-p using Δγ correlator w.r.to \Psi_1"


Slide#14:
remove "too large to conclude"

Slide#3:
"We need better method"
-->
"We need a better method"




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