STAR Flow, Chirality and Vorticity PWG

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

Dear Gavin,

I mean to remove the line 117.
For the fit in the Figure, I am fine with it either ways.

Thanks and regards,
Subhash

On 2024-01-19 09:35 PM, Gavin Wilks wrote:
> Dear Subhash,
>
> Thank you for the comments.
>
> Regarding your comment on line 117, are you suggesting that I remove
> the fit to BES-I data in the figure?
>
> Best,
> Gavin
>
> > On Jan 19, 2024, at 04:16, subhash via Star-fcv-l 
> > <star-fcv-l AT lists.bnl.gov> wrote:
> >
> > Dear Gavin,
> >
> > Very nice proceedings. I have a few questions and suggestions below 
> > for your consideration:
> >
> > abstract:
> > s = s_NN =
> > nuclear structure --> What do you mean by nuclear structure here, I 
> > didn't get the context here.
> >
> > l#10: At the center of non-central --> At the non-central
> > l#25: rest frame
> > l#43-44: Along this line, you may mention BES-II allow more precision 
> > and differential measurements which were not possible from BES-I.
> > l#61: some temporary complications of signal extraction --> I think 
> > this line is not needed, since it do not explain what is the 
> > underlying complication. It seems too technical.
> > Or may be you can rephrase something like, In future we will extend 
> > measurements beyond 1.0 !
> > l#68:  The mixed-event method is used to generate the combinatorial 
> > background ....
> > l#72-73: Have you varied background shape eg poly-3 vs poly-2 for 
> > systematics?
> > l#75: Is the width fixed to PDG or extracted from data for integrated 
> > theta* bins?
> > l#94-95: Do you apply any PID efficiencies?
> > l#115: The fit presented for the second-order event plane results is s 
> > fit only to BES-I
> > --> may be rephrased as, the solid line is a fit only to BES-I data 
> > ...
> > l#117: The BES-II data at √𝑠NN = 19.6 GeV is consistent with the model 
> > fit from BES-I and the details of the fit can be found in [1].
> > --> I think this line is not necessary and can be removed. A better 
> > approach would be to fit when precise data will be available for all 
> > BES-II energies.
> > l#153:  to be more specific: ... increasing 𝜌00 with rapidity 
> > (|y|>0.5) for both energies ...
> > l#156:  many collision energies --> remaining collision energies
> > l#157: I'd suggest a rephrase: This work explores the potential link 
> > between the 𝜙-meson field and global spin alignment, ....
> >
> >
> > I sign off with these addressed.
> >
> > Thanks and regards,
> > Subhash
> >
> >
> > On 2024-01-19 01:52 AM, webmaster--- via Star-fcv-l wrote:
> > > Dear star-fcv-l AT lists.bnl.gov members,
> > > Gavin Wilks (gwilks3 AT uic.edu) has submitted a material for a review, 
> > > please
> > > have a look:
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