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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Gavin Wilks for SPIN 2023 submitted for review

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: Gavin Wilks <gwilks3 AT uic.edu>
  • To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Gavin Wilks for SPIN 2023 submitted for review
  • Date: Fri, 19 Jan 2024 14:35:47 +0100

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:
>> https://urldefense.com/v3/__https://nam04.safelinks.protection.outlook.com/?url=https*3A*2F*2Fdrupal.star.bnl.gov*2FSTAR*2Fnode*2F66594&data=05*7C02*7Cgwilks3*40groute.uic.edu*7Cb2629a325f8641ee1e6908dc189d1881*7Ce202cd477a564baa99e3e3b71a7c77dd*7C0*7C0*7C638412310220337425*7CUnknown*7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0*3D*7C3000*7C*7C*7C&sdata=IqE7otOr3JjFMqEmlVvr4Ux17ehaQXAPt*2F3IGK*2FRH7c*3D&reserved=0__;JSUlJSUlJSUlJSUlJSUlJSUlJSUlJSUl!!P4SdNyxKAPE!AuzVYRJqyJIzMep7tJe8jOQgxbpx8WF2-j8cHQmQGYzsvfH7JmMIEbfv5AxkEqwbFnb0d5w4zAjUU1_MYugK4y4n$
>>
>> ---
>> If you have any problems with the review process, please contact
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