STAR Flow, Chirality and Vorticity PWG

[subhash <subhash AT rcf.rhic.bnl.gov>]

Dear Prabhupada,

Thanks for considering the suggestions. I have a few additional minor 
ones for your consideration:

In general
for math-symbols, please use \mathrm, e.g for \phi \mathrm{weight}
error bars --> uncertainties

line 20: please mention upgrade of inner TPC.
line 31: you could mention improvement in EP resolution compared to 
BES-I
line 52: for all particles (left) and antiparticles (right), 
respectively.


Fig1 caption: Mention using TPC and iTPC

Other Fig. Captions:
uncertainty --> uncertainties.
The vertical lines and caps represent the  statistical and systematic 
uncertainties.
remove "is plotted"
The plot on the left --> Left figure
Lower left panel and so on ...
(same suggestions for relevant captions)

Thanks and regards,
Subhash

On 2022-10-17 10:36 AM, pdixit via Star-fcv-l wrote:
> Dear Subhash,
> The link to the latest version of the proceeding is
> https://drupal.star.bnl.gov/STAR/system/files/ICHEP_proceedings_v3.pdf
> after a small correction in the typo.
>
> Regards,
> Prabhupada
> On 2022-10-17 10:17, pdixit via Star-fcv-l wrote:
> > Dear Subhash,
> > Thank you for the comments and suggestion. The corrected version of
> > the proceeding can be found in the link below. Please have a look.
> > https://drupal.star.bnl.gov/STAR/system/files/ICHEP_proceedings_v2.pdf
> >
> > Regards,
> > Prabhupada
> > On 2022-10-16 09:02, subhash via Star-fcv-l wrote:
> > > Dear Prabhupada,
> > >
> > > Nice proceedings. I have a few suggestions for your consideration:
> > >
> > > abstract: add a space between KS0 and Lambda
> > > remove 14.6. You are not showing anything from this energy.
> > > The hydrodynamically motivated ratio ... is presented as a function 
> > > of pT
> > >
> > > line 11: If Psi_n is event plane here, then you need resolution 
> > > factor
> > > in equation 2
> > >
> > > line 13: remove initial
> > >
> > > line 16-17: To overcome this problem, --> I don't understand the
> > > problem here. I think you mean multi-strange hadrons are not affected
> > > by late stage hadronic rescattering. Could you rephrase the sentence.
> > >
> > > line 19: You could elaborate/specify on the detector upgrades and
> > > increase in number of events here.
> > >
> > > line 24-26: I think the "𝜙 − 𝑤𝑒𝑖𝑔ℎ𝑡" is the inverse of dN/d𝜙 right.
> > > First define it then say it is used to flaten the event plane.
> > >
> > > line 26-27: Please rephrase it.
> > >
> > > line 28: Add the the eta regions of sub-events?
> > >
> > > line 35:  particles and anti-particles --> Mention particle species 
> > > here.
> > >
> > > line 48: define what is modified ncq here
> > >
> > > line 53: this could be due to the effect from transported quarks
> > >
> > > line 61: weak dependence on pT above 1.5 GeV/c
> > >
> > > line 68: because its dominant cause is --> may be due to the initial
> > > eccentricity  ....
> > >
> > > line 70:  because its main cause -->  because it is expected from the
> > > event-by-event fluctuation ....
> > >
> > > line 72: which can be attributed to ...
> > >
> > >
> > > I sign off with these addressed.
> > >
> > >
> > > Thanks and regards,
> > > Subhash
> > >
> > >
> > > On 2022-10-11 03:34 AM, webmaster--- via Star-fcv-l 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/61286
> > > >
> > > > ---
> > > > If you have any problems with the review process, please contact
> > > > webmaster AT www.star.bnl.gov
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