STAR HardProbes PWG

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

Hello Yuan,

Thank you for implementing my comments.
Here is an additional comment. With this implemented, I sign off.

L73:	In this work, the minimum bias datasets are collected in Au+Au 
collisions at √sNN = 200 GeV in the year 2014.
 -> In this analysis, the minimum bias Au+Au collisions at √sNN = 200 
GeV data, taken in the year 2014, is used.


Best
Nihar

On 2023-12-04 22:41, suyuann AT mail.ustc.edu.cn wrote:
> Hi Nihar,
>
> Thanks a lot for your nice comments, please find the update version:
> https://drupal.star.bnl.gov/STAR/node/66071
>
> Best regards,
> Yuan
>
>
> > -----原始邮件-----
> > 发件人: "Nihar Sahoo" <nihar AT rcf.rhic.bnl.gov>
> > 发送时间: 2023-12-04 11:43:37 (星期一)
> > 收件人: suyuann AT mail.ustc.edu.cn
> > 抄送: "STAR HardProbes PWG" <star-hp-l AT lists.bnl.gov>, 
> > webmaster AT star.bnl.gov
> > 主题: Re: [Star-hp-l] STAR presentation by Yuan Su for Quark Matter 2023 
> > submitted for review
> >
> > Hello Yuan,
> >
> > Please find my comments on your nice proceedings.
> >
> > L7: We report the first measurements of.. -> We report the 
> > measurements
> > of…
> > _     transverse momentum pT -> transverse momentum (pT)
> > L11:  modification factor RAA is observed -> modification factor is
> > observed
> > L14:  in 200 GeV Au+Au collisions ->  in √sNN = 200 GeV at Au+Au
> > collisions
> >   L14-17: "We show the nuclear modi- fication factor RCP of D0-tagged
> > jets as a function of pT,Jet and zJet. Additionally, the radial 
> > profile
> > of the D0 mesons in these tagged jets are obtained with 1 < pT,D0 < 10
> > GeV/c for different centrality classes." -> Let's concise it.
> > "we present the nuclear modification factor and radial profile of
> > D^0-tagged jets with 1 < pT,D0 < 10 GeV/c. "
> >
> > L22: They are expected to suffer… ->They lose energy due to 
> > interactions
> > with the medium; hence studying heavy quark in heavy-ion collisions 
> > can
> > shed light on the QGP properties.
> >
> > L24: …modification factor RAA was …-> …modification factor, RAA, was …
> > L32: you need to mention what are these pT,hadron, and pTjet are in z?
> > L36:.  …jets can help constrain theoretical … -> … jets can help to
> > constraint the theoretical…
> >                 parton mass and -> parton mass, and
> > L38-40: In this proceedings,… -> These lines are needed, in stead you
> > can discuss more on the topics.
> > L44: are directly used -> are used
> > L48: in the 200 GeV isobar collisions -> in isobar collisions at
> > \sNN=200 GeV
> >
> > L49.	Figure  1. -> Fig.1 [Elsewhere inside the sentence; L58, L66, 
> > L71,
> > L84, L89]
> > L50: at 200 GeV -> at \sNN=200 GeV; Mention what is <N_bin>?
> > L51:	Vertical lines and … , respectively. ->  remove this sentence 
> > here
> > and include in the caption of Fig.1
> > L52-53:The generally consistent indicates that the D^0… -> The D^0
> > production …
> >
> > L55: Levy fits -> the Levy fit; "… GeV/c and plotted by dot lines. " 
> > ->
> > "… GeV/c." remover rest. [data point description you can put in the
> > caption]
> > L56: And D0 yields in …by solid lines. -> Remove this sentence, not
> > needed.
> > L60:    …collisions has an obvious suppression effect … -> …collisions
> > show suppression at pT > 3 GeV/c,..
> > L62: Mention and cite the model predictions.
> > Figure 2 caption: Blast-Wave fits -> the Blast-wave fits
> > L64: inverse slope parameter Teff  -> inverse slope parameter, Teff,
> > L65: in 200 GeV -> in \sNN = 200 GeV
> > L67: 		the singular and charm hadrons -> what is "singular" here?  
> > This
> > sentence is not clear.
> > L71: present BW fit -> present the Blast-wave fit
> > kinetic freeze-out temperature Tkin -> kinetic freeze-out temperature,
> > Tkin,
> > L71-73: This entire sentence is not needed. And Not clear .
> > L75-76:         …a similar dynamic process in the bulk medium with respect to
> > Au + Au collisions. -> Not clear, please rephrase
> > L79:    The data sets in this work… ->  In this work, the minimum bias
> > datasets are collected in Au+Au
> > L80: from RHIC run year 2014. -> in the year 2014.
> > L82: Rcp: mention centralities
> > L87: …          the D0 tagged jet invariant yields in peripheral, but
> > underestimates in central collisions. -> No figure is included in this
> > proceedings. Right?
> > L88: what is TAA? Mention it.
> > L89: zJet: here this is different notation compared with L32; make it
> > consistent
> > L95: LIDO model (MPI = off) … -> The LIDO model 	() describes the 
> > ratio
> > of radial profile in the data.
> > … mention what is MPI
> > L98: To summarize, we reported … -> We report
> > L102:           while light hadrons may be -> Either remove this or mention
> > "while light hadrons show negligible difference."
> > L102:And the strong suppression of D0 nuclear modification factor RAA 
> > is
> > -> The strong suppression of D0 nuclear modification factor is
> > L104: D^0 tagged jet suppression
> >
> >
> > Best
> > Nihar
> >
> > On 2023-12-03 20:16, suyuann AT mail.ustc.edu.cn wrote:
> > > Hi Nihar,
> > >
> > > Thank you for your comment. Please find the update version:
> > > https://drupal.star.bnl.gov/STAR/node/66071
> > >
> > > Best regards,
> > > Yuan
> > >
> > >
> > >> -----原始邮件-----
> > >> 发件人: "Nihar Sahoo via Star-hp-l" <star-hp-l AT lists.bnl.gov>
> > >> 发送时间: 2023-12-04 01:09:27 (星期一)
> > >> 收件人: "STAR HardProbes PWG" <star-hp-l AT lists.bnl.gov>
> > >> 抄送: "Nihar Sahoo" <nihar AT rcf.rhic.bnl.gov>, webmaster AT star.bnl.gov
> > >> 主题: Re: [Star-hp-l] STAR presentation by Yuan Su for Quark Matter 2023
> > >> submitted for review
> > >>
> > >> Hello Yuan,
> > >>
> > >> Can you please add line numbers in your proceedings?
> > >> It helps.
> > >>
> > >> Thank you
> > >> Nihar
> > >>
> > >>
> > >> On 2023-11-23 21:10, webmaster--- via Star-hp-l wrote:
> > >> > Dear Star-hp-l AT lists.bnl.gov members,
> > >> >
> > >> > Yuan Su (suyuann AT mail.ustc.edu.cn) has submitted a material for a
> > >> > review,
> > >> > please have a look:
> > >> > https://drupal.star.bnl.gov/STAR/node/66071
> > >> >
> > >> > ---
> > >> > If you have any problems with the review process, please contact
> > >> > webmaster AT www.star.bnl.gov
> > >> > _______________________________________________
> > >> > Star-hp-l mailing list
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