STAR HardProbes PWG

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

Hello Gabe,

Thank you for implementing my comments.
It reads good in the current form. I sign off.


> I intentionally left details out on the constituent cut and jet radius
> in the original draft, because I didn’t want to clutter the abstract
> with too much detail. I can leave them in if you prefer. Also I would
> prefer a more nuanced discussion of the effects of varying jet-R, but
> I feel this is also too much for the abstract. For now I put one
> sentence in justifying the method, but I feel it is over simplified,
> and would be better as a discussion in the talk. Let me know if you
> have any other input on how much to include in terms of discussing
> “why it is important”.

This can be addressed in your presentation. So never mind now.

Best
Nihar


On 2024-05-15 01:36, Gabe Dale-Gau wrote:
> Hello Nihar,
>
> Thank you for your comments.
>
> I have updated the submission page with a new version of the abstract.
> Individual responses to your comments are listed below.
>
> Thanks,
>
> Gabe
>
> 1_ baryon-to-meson yield ratios -> baryon-to-meson inclusive hadron
> yield ratios [Need to mention this because to avoid "in-jet
> baryon-to-meson ratio" and "baryon-to-meson inclusive hadron yield
> ratio"]
>
> Good point. Implemented as suggested.
>
> 2_ jet-track correlation -> jet-charged hadron correlation or simply
> "jet-hadron correlation"
>
> Implemented as suggested.
>
> 3_ "…jet radii and jet constituent pT selections. " -> You need to
> pointed out that this abstract will cover results from pT>2.0GeV/c and
> what jet R. Which is new and important for this measurement. You need
> also to highlight why it is important to have a measurement pT>2 GeV/c
> and different jet R?
> Otherwise, this abstract reads similar to previous years' abstract.
>
> Updated to the following:
>
> “these in-jet ratios are studied as a function of jet radii, R $=
> 0.2, 0.3, 0.4$, and jet constituent $p_{\rm{T}}$ selections,
> $p^{\rm{const}}_{\rm{T}} > 2.0$ GeV/$c$, $3.0$ GeV/$c$. Varying the
> jet radius and constituent $p_{\rm{T}}$ selection allows us to probe
> jets with different levels of QGP interaction.”
>
> I intentionally left details out on the constituent cut and jet radius
> in the original draft, because I didn’t want to clutter the abstract
> with too much detail. I can leave them in if you prefer. Also I would
> prefer a more nuanced discussion of the effects of varying jet-R, but
> I feel this is also too much for the abstract. For now I put one
> sentence in justifying the method, but I feel it is over simplified,
> and would be better as a discussion in the talk. Let me know if you
> have any other input on how much to include in terms of discussing
> “why it is important”.
>
> On Tue, May 14, 2024 at 7:13 AM Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
> wrote:
>
> > Hello Gabe,
> >
> > Please find my comments on your abstract.
> >
> > 1_ baryon-to-meson yield ratios -> baryon-to-meson inclusive hadron
> > yield ratios [Need to mention this because to avoid "in-jet
> > baryon-to-meson ratio" and "baryon-to-meson inclusive hadron yield
> > ratio"]
> >
> > 2_ jet-track correlation -> jet-charged hadron correlation or simply
> >
> > "jet-hadron correlation"
> >
> > 3_ "…jet radii and jet constituent pT selections. " -> You need to
> >
> > pointed out that this abstract will cover results from pT>2.0GeV/c
> > and
> > what jet R. Which is new and important for this measurement. You
> > need
> > also to highlight why it is important to have a measurement pT>2
> > GeV/c
> > and different jet R?
> > Otherwise, this abstract reads similar to previous years' abstract.
> >
> > Best
> > Nihar
> >
> > On 2024-05-10 19:44, Gabe Dale-Gau via Star-hp-l wrote:
> > > Dear HP-conveners,
> > >
> > > I would like to highlight the final sentence of this abstract, "
> > These
> > > in-jet ratios are studied as a function of jet radii and jet
> > > constituent pT selecitons. ", to point out the difference between
> > what
> > > I am submitting this year and what I presented last year. This
> > year,
> > > with a more developed method for correlated background removal, I
> > plan
> > > to present results for constituent pT > 2.0 GeV/c, and using the
> > > increase in statistics that comes along with this jet sample, I
> > plan
> > > to present a radial study of the p/pi ratios as well.
> > >
> > > Thanks,
> > >
> > > Gabe
> > >
> > > On Fri, May 10, 2024 at 8:40 AM webmaster--- via Star-hp-l
> > > <star-hp-l AT lists.bnl.gov> wrote:
> > >
> > > > Dear Star-hp-l AT lists.bnl.gov members,
> > > >
> > > > Gabriel Dale-Gau (gdaleg2 AT uic.edu) has submitted a material for a
> > > > review,
> > > > please have a look:
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> > [1]
> > > > [1]
> > > >
> > > > Deadline: 2024-05-25
> > > > ---
> > > > If you have any problems with the review process, please contact
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> > [2]
> > > > [2]
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> [6] 
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