STAR Flow, Chirality and Vorticity PWG

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

Dear Takafumi
Thanks for the nice presentation, I would approve with a few minor comments. 

* You have mentioned about the update on the alpha parameter in p4 between 
old and new results, 
but the update has been applied only for the p22-25, right? So it might be 
easier for the audience 
to follow, if you mention these changes when you show these a few figures. 
But since the parameters 
are printed only on these new figures, so it would already be clear enough… 

* on p2, I see some overlapping words on the left-bottom of the page, which 
might be my viewer
problem as well, though.  

* It would be nice, if you can also discuss about your BW calculations in 
your talk from the backup 
slides p35-36. Have you also made your own calculation with your BW 
assumption for the azimuthal 
dependent gPh measurement on p18? 

Best regards, ShinIchi

PS : I do see overlapping posts for the same Petr’s ICPPA proceedings from 
Grigory and Arkadiy, 
so I wonder which one I should be reading. Do you know? Petr should be 
posting to avoid this confusions.  

> On Oct 12, 2020, at 1:16, webmaster--- via Star-fcv-l 
> <star-fcv-l AT lists.bnl.gov> wrote:
> 
> Dear star-fcv-l AT lists.bnl.gov members,
> 
> Takafumi Niida (taknda AT hotmail.co.jp) has submitted a material for a 
> review,  
> please have a look:
> https://drupal.star.bnl.gov/STAR/node/52333
> 
> ---
> 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