STAR Flow, Chirality and Vorticity PWG

[ShinIchi Esumi <esumi.shinichi.gn AT u.tsukuba.ac.jp>]

Dear Prabhupada
Thanks for the very nice proceeding, I would sign off with some minor comments
for you to consider in the followings. 

L58 : comma “,” just before the “so”.
L77(and Fig.2) : It looks like you used the data points as a part of the 
fitting function, 
which is good, I would just like to suggest you to include the Minv 
distribution 
(without subtraction) overlaid with normalized mixed BG, just above the 
v2(Minv) 
plot with exactly the same x axis (the same Minv region) and to state S,B in 
the 
fitting function are given by data points (therefore the fitted line includes 
the 
statistical fluctuation from the S and B). 
Fig.4 : Since you always present 27 and 54 GeV data separately, I would 
overlay 
them at lease once, which could be done in this Fig.4, or at least, to have 
them 
separately as it is now, but choose exactly the same x-y scale of the figure 
and 
add the grid lines in the figure, since I would also like to see the 
comparison between 
two energies, for both data and ampt. Why did you choose to use 3mb (default 
value 
in ampt)?, where I remember data are better described with somewhat larger 
partonic 
cross section at lease for higher energies. 
Best regards, ShinIchi

> On Feb 9, 2021, at 3:10, webmaster--- via Star-fcv-l 
> <star-fcv-l AT lists.bnl.gov> wrote:
> 
> Dear star-fcv-l AT lists.bnl.gov members,
> 
> Prabhupada Dixit (prabhupadad AT iiserbpr.ac.in) has submitted a material for 
> a  
> review, please have a look:
> https://drupal.star.bnl.gov/STAR/node/53631
> 
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