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  • From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
  • To: Star-hp L <Star-hp-l AT lists.bnl.gov>
  • Cc: STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
  • Subject: Re: [Star-hp-l] STAR jet acoplanarity paper draft; request to form GPC
  • Date: Tue, 18 Jun 2024 13:55:05 +0530

Hello Rongrong, Yi , and Isaac,

Thank you for your constructive comments.

We have worked on your comments. Please find our responses at one place:
(Rongrong, Yi, and Isaac's comments are in order)
https://drupal.star.bnl.gov/STAR/system/files/PWGComments_Acoplanarity_June16.pdf

In this revised paper draft, Supplement material is included.
Revised paper draft (v2):https://drupal.star.bnl.gov/STAR/system/files/AcoplanarityPaper_v2.pdf
Revised AN v2: https://drupal.star.bnl.gov/STAR/system/files/AcoplanarityAanalysisNote_V2_0.pdf

We request HP-pwg converners to help us forming GPC.

Best
Nihar for PAs( Derek, Saskia, Peter)



On 2024-05-06 12:55, Yi Yang wrote:
Hi Nihar,

Thanks a lot for the well-written draft and analysis note.
I agree with Rongrong's comments, so won't repeat here. I have some
minor ones for your consideration.

Paper draft:
- L36 - 38: the hyphens look a bit strange to me, it should look
like the one in L26. (similar for L314 and 315)
- L41: high energy --> high-energy
- L58: pT, jet > 30 GeV/c
- L59: R=0.3 --> R = 0.3
- L116: Gev --> GeV
- Eq.(1) and (2): it should be d^2 N_jet and d^2 sigma
- L156: sqrt(s_NN)=200 GeV --> sqrt(s_NN) = 200 GeV
- Figure 1: I would suggest to put the information in the right
panel to the left panel as well, just in case someone cut the left
panel only and there is no information on that.
- L229: What does "TBD" mean here? Will this affect the final
physics conclusion?
- L245: Fig.2 --> Figure 2

Question: (I probably asked it earlier) you show different behavior
for R = 0.2 and 0.5, does it make sense to try other R numbers to see
the actual R-dependence?

Analysis note:
- L172: Figure 23 --> Figure 9?
- Question: you are using PYTHIA-8 in the embedding/simulation, but
you used PYTHIA-6 for the comparison in the result. Why not use the
same version of PYTHIA?
- Don't you have the systematics from the unfolding iteration?
- Figure 23: It clearly shows the closure is not good between 2.5
and 3, and you are using log in the ratio. Any systematics associated
with it?
- L403, 404: there are "TBA"s, what does that mean?
- L435: The uncertainty on dPhi weights is "TBD"?
- Figure 26: do you have a similar plot for R = 0.2? What do the two
"light blue" lines mean here?

Cheers,
Yi

On Mon, Apr 8, 2024 at 10:16 AM Nihar Sahoo via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:

Hello HP-pwg,

We have finalized STAR gamma+jet and pi0+jet acoplanarity paper
draft.
Paper draft, analysis Note, and paper webpage can be found below.
Please send your comment and feedback.
We request to form GPC.

Paper draft:

https://drupal.star.bnl.gov/STAR/system/files/AcoplanarityPaper_v1.pdf

Analysis Note:

https://drupal.star.bnl.gov/STAR/system/files/AcoplanarityAanalysisNote_V0_0.pdf

Paper webpage:

https://drupal.star.bnl.gov/STAR/blog/nihar/Paper-webpage-Measurement-direct-photonjet-and-pi0jet-azimuthal-correlation-AuAu-and-pp-c

Thank you
PAs (Nihar, Derek, Saskia, and Peter)

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