STAR HardProbes PWG

[Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>]

Hello Yan,

Thank you for addressing my comments.
I sign off

Cheers
Nihar

On 2023-03-19 12:02, wy157543 AT mail.ustc.edu.cn wrote:
> Hi, Nihar
>
> Thank you for your nice comments. New version can be found in this 
> link:
> https://drupal.star.bnl.gov/STAR/system/files/HP_v4_0.pdf
> "Red vertical upward arrow" mean debey radius reduce with temperature 
> increase.
> Isobar RAA at 60-80% close to 1.so we think no significant suppression
> and pT depedence is observed.
>
> best,
> Yan
>
> > -----原始邮件-----
> > 发件人: "Nihar Sahoo" <nihar AT rcf.rhic.bnl.gov>
> > 发送时间: 2023-03-18 17:25:12 (星期六)
> > 收件人: wy157543 AT mail.ustc.edu.cn, "STAR HardProbes PWG" 
> > <star-hp-l AT lists.bnl.gov>
> > 抄送: webmaster AT star.bnl.gov
> > 主题: Re: [Star-hp-l] STAR presentation by Yan Wang for Hard Probes 2023 
> > got commented by Xin Dong
> >
> > Hello Yan,
> >
> > Thank you for your nice comments.
> > Please find my comments below.
> >
> > Slide-3:
> > "Jet quenching" -> Since you are discussing on J/psi so jet quenching
> > may not relevant. You could mention "J/psi suppression"
> >
> > In the top cartoon, what does "Red vertical upward arrow" represent
> > there along with "T"?
> >
> > Slide-4
> > "All these effects are expected to strongly depend on collision system
> > size " -> "All these effects are expected to show strong dependence on
> > collision system size"
> >
> > Slide-6:
> > Please increase the X,Y-axis title size.
> >
> > SLide-8:
> > Sorry, I have not followed this before.
> > Could you inform me what does "Isobar, 60-80%" represent in RAA plot?
> >
> >
> > Slide-14:
> > "Indicate that the color-screening effect is dominant in isobaric
> > collisions"
> > I think you could add this "color-screening effect" in one of 
> > Silde8,9;
> > Although you have mentioned suppression but if you could add
> > "Significant suppression observed at large Npart due to 
> > color-screening
> > effect" (in SLide9) then it would be good to say at the end.
> >
> >
> > Cheers
> > Nihar
> >
> >
> >
> >
> >
> >
> > On 2023-03-17 08:17, wy157543--- via Star-hp-l wrote:
> > > Hi Xin Dong,
> > >
> > >   Thanks for your comments, I will update the figure later.
> > > I am sorry for the link issue, the slide can be found in this link:
> > > https://drupal.star.bnl.gov/STAR/system/files/HP_v2_2.pdf
> > >
> > > best,
> > > Yan
> > >
> > >
> > >
> > >> -----原始邮件-----
> > >> 发件人: "webmaster--- via Star-hp-l" <star-hp-l AT lists.bnl.gov>
> > >> 发送时间: 2023-03-17 05:31:13 (星期五)
> > >> 收件人: Star-hp-l AT lists.bnl.gov
> > >> 抄送:
> > >> 主题: [Star-hp-l] STAR presentation by Yan Wang for Hard Probes 2023 got
> > >> commented by Xin Dong
> > >>
> > >> Dear Star-hp-l AT lists.bnl.gov members,
> > >>
> > >> Xin Dong ( xdong AT lbl.gov ) has commented on a material originally
> > >> submitted
> > >> by Yan Wang ( wy157543 AT mail.ustc.edu.cn ) at
> > >> 
> > https://drupal.star.bnl.gov/STAR/presentations/Hard-Probes-2023/Jpsi-production-RuRu-and-ZrZr-collisions-200GeV-STAR-experiment
> > >>
> > >> Comment:
> > >> Hi Yan, it looks like the link below doesn't work. But I managed to
> > >> access it
> > >> by changing the filename to "HP_v2_0.pdf" (believe it is the current
> > >> draft).
> > >> I have one suggestion to your nice result in slide 13. I think it
> > >> would be
> > >> better to add the D0 v2 data points together to better illustrate the
> > >> conclusion you have on the slide "limited regeneration". Thanks /xin
> > >>
> > >> ---
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> > >> webmaster AT www.star.bnl.gov
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