STAR Flow, Chirality and Vorticity PWG

[Jiangyong Jia <jiangyong.jia AT stonybrook.edu>]

Hi, Niseem,

The poster looks great.   Just a few comments

1 Have you done the two checks that were suggested during the
preliminary request?  please circulate those to the list.
a) Check the pT spectra to make sure the shapes are similar to published
one.
b) High-pT Dphi correlation function for AuAu and pp region to make sure
the shape in dPhi looks reasonable before and after the subtraction.

2 It is not clear to me it is useful to put the abstract in the poster,
since the poster presents the results and have a conclusion section already

3 For system-size result, since you shown things up to 9 GeV, I would
remove the x-axis range above 9 GeV

4 It would be good to provide some details about the Glauber model you
used to calculate the epsilon_2, since the result may depend on the
setup of the Glauber

Jiangyong
On 1/1/21 4:58 PM, webmaster--- via Star-fcv-l wrote:
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Niseem Magdy Abdelwahab Abdelrahman (niseemmagdy AT yahoo.com) has submitted a 
>  
> material for a review, please have a look:
> https://drupal.star.bnl.gov/STAR/node/53176
>
> ---
> If you have any problems with the review process, please contact  
> webmaster AT www.star.bnl.gov
> _______________________________________________
> Star-fcv-l mailing list
> Star-fcv-l AT lists.bnl.gov
> https://lists.bnl.gov/mailman/listinfo/star-fcv-l