STAR Flow, Chirality and Vorticity PWG

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

Dear Shuai,

Thanks for incorporating my suggestions. I have a few additional ones:

General: Please check X/Y-axis labels is hidden behind figures/frames
It would be good if X/Y axis label sizes are increased.
In several places, 14.6 GeV instead of 14.6GeV

s3: pressure gradient and interaction among ... FINAL ...
Please add reference to flow papers

s5: Sub-event method
You could mention event plane is a proxy for reaction plane

s6: left plot title: TPC Event plane
right plot:  remove ZS in legend
second bullet: v_2

s7: Add a reference to STAR papers, where such rotations are applied

s9: protons are identified ... up to pt 3.2 GeV/c
Remove the statistical boxes inside figures.

s12 & 13: Instead of squeezing two plots, you can probably animate them 
one by one with a larger size of figure.

In one of the v2 slide, or in summary you can probably mention the 
reduction of errors in BES-II compared to BES-I.

I sign off once these are addressed.


Thanks and regards,
Subhash






On 2022-11-26 03:59 PM, zs155167 wrote:
> Dear conveners,
>
>    I have updated my slide for CPOD2022. Please have a look at the new
> version here:
>
> https://drupal.star.bnl.gov/STAR/system/files/CPOD2022_Shuai_Zhou_1.pdf
>    If you have any comments and suggestions, please let me know. Thank
> you very much!
>
> Best and regards,
> Shuai Zhou
>
> ------------------ Original ------------------
>
> From:  "周帅"<zs155167 AT mails.ccnu.edu.cn>;
> Date:  Wed, Nov 23, 2022 09:00 PM
> To:  "subhash"<subhash AT rcf.rhic.bnl.gov>; "STAR Flow,Chirality
> and"<star-fcv-l AT lists.bnl.gov>;
>
> Subject:  Re: [Star-fcv-l] STAR presentation by Shuai Zhou for CPOD
> 2022 submitted for review
>
>  Dear Subhash,
>
>  Thanks for your comments and suggestion. Here are my illustrations:
>
> For the new BES-II 14.6 GeV pi, K, p v2 data, do you have a comparison
> with BES-I that we can take a look?
>
>  Yes, please find my slide here:
> https://drupal.star.bnl.gov/STAR/system/files/v2ratio.pdf [1]
>
> I see, you have presented individual pi, K, p v2 at FCV, but I feel
> that
> the NCQ scaling results especially on slide 12 and 13 are new. Could
> you
> discuss it today at the FCV?
>
> OK, I will illustrate it today at the FCV
>
> Do you observe any centrality dependence in NCQ scaling behavior?
>
> Within errors, no obvious centrality dependence is observed.
>
> Is it possible to make a single NCQ scaling plot, including all
> particles measured. I mean pi, K, p (from you) and multi-stranges from
> Prabhupada.
>
>   OK, I will contact Prabhupada about this.
>
>  There was some discussions at the FCV related to the
> asymmetricmass-square selection. Could you indicate if you have done
> any check?
>
> Yes, I have checkd it, please find:
> https://drupal.star.bnl.gov/STAR/system/files/star_prelimilary_update.pdf
> [2]
>
> Please include, collision system, energy, TPC+iTPC etc within the
> figure
> where these informations are missing; Add X and Y-axis labels etc.
>
> s4: last bullet: identification using m2
>
> s6: For resolution plot, it would be good to comparison with BES-I
>
> s10, 11: Could you increase legends size
>
> Yes, I will improve it
>
> ------------------ Original ------------------
>
> From:  "subhash"<subhash AT rcf.rhic.bnl.gov>;
> Date:  Wed, Nov 23, 2022 05:43 PM
> To:  "周帅"<zs155167 AT mails.ccnu.edu.cn>; "STAR Flow,Chirality
> and"<star-fcv-l AT lists.bnl.gov>;
>
> Subject:  Re: [Star-fcv-l] STAR presentation by Shuai Zhou for CPOD
> 2022 submitted for review
>
> Dear Shuai,
>
> Thanks for reminder. I have a few comments and suggestions.
>
> General:
> For the new BES-II 14.6 GeV pi, K, p v2 data, do you have a comparison
>
> with BES-I that we can take a look?
>
> I see, you have presented individual pi, K, p v2 at FCV, but I feel
> that
> the NCQ scaling results especially on slide 12 and 13 are new. Could
> you
> discuss it today at the FCV?
>
> Do you observe any centrality dependence in NCQ scaling behavior?
>
> Is it possible to make a single NCQ scaling plot, including all
> particles measured. I mean pi, K, p (from you) and multi-stranges from
>
> Prabhupada.
>
> There was some discussions at the FCV related to the asymmetric
> mass-square selection. Could you indicate if you have done any check?
>
> Please include, collision system, energy, TPC+iTPC etc within the
> figure
> where these informations are missing; Add X and Y-axis labels etc.
>
> s4: last bullet: identification using m2
>
> s6: For resolution plot, it would be good to comparison with BES-I
>
> s10, 11: Could you increase legends size
>
> Thanks and regards,
> Subhash
>
> On 2022-11-23 02:11 PM, zs155167 via Star-fcv-l wrote:
> > Dear convenors,
> >
> >  I have submitted my slides for CPOD 2022. If you have any
> suggestion
> > or comments, please let me know. Thank you!
> >
> > Best regards,
> > Shuai Zhou
> >
> > ------------------ Original ------------------
> >
> > From:  "STAR Flow,Chirality and"<star-fcv-l AT lists.bnl.gov>;
> > Date:  Mon, Nov 21, 2022 04:18 PM
> > To:  "STAR Flow,Chirality and"<star-fcv-l AT lists.bnl.gov>;
> >
> > Subject:  [Star-fcv-l] STAR presentation by Shuai Zhou for CPOD 2022
> > submitted for review
> >
> > Dear star-fcv-l AT lists.bnl.gov members,
> >
> > Shuai Zhou (zs155167 AT mails.ccnu.edu.cn) has submitted a material for
> a
> > review, please have a look:
> > https://drupal.star.bnl.gov/STAR/node/61798
> >
> > Deadline: 2022-11-28
> > ---
> > 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
> > _______________________________________________
> > Star-fcv-l mailing list
> > Star-fcv-l AT lists.bnl.gov
> > https://lists.bnl.gov/mailman/listinfo/star-fcv-l
>
>
> Links:
> ------
> [1] https://drupal.star.bnl.gov/STAR/system/files/v2ratio.pdf
> [2] 
> https://drupal.star.bnl.gov/STAR/system/files/star_prelimilary_update.pdf