STAR HardProbes PWG

[Sooraj Radhakrishnan <skradhakrishnan AT lbl.gov>]

Hi Tanmay,

    I believe you are showing the plots on S7 as a work in progress. Please indicate on the plots these are uncorrected distributions. Also it would be better not to draw any physics observations from these plots. You could say have good statistical precision to measure in different pT bins. The hard core constituent cut is not described anywhere, I believe the point is the discontinuous distribution is from jets with different number of tracks with the hard core requirement coming in. May be this can be described better than how its now.

thanks

Sooraj

On Mon, Oct 17, 2022 at 12:37 PM Nihar Sahoo via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

Hello Tanmay,

Can you please remind me if your analysis's results are already "STAR
preliminary" or this is first time?

Please find my comments on your nice presentation slides.

SLide1:
Title: "Jet Shape Observables at √sNN = 200 GeV in RHIC" -> "Jet Shape
Observables in p+p Collisions at √s = 200 GeV in STAR"
(As you are showing here only pp results, that would be fine)

Slide2:
_ w.r.t.  -> relative to
_probes to study QGP  -> probes to study QGP properties
_Experimentally, jets ….-> Remove this bullet, not required.
_Jets reconstructed from tracks and tower energy depositions using the
FASTJET library ->      Jet reconstruction using charged tracks and
calorimeter tower energy depositions by anti-kT algorithm (Give
reference of FASTJET/anti-Kt)

Slide3:
_ …, e.g. π0, γ, etc.-> …, e.g., pi0, electron, etc. (as in your full
jet we don't consider any gamma inside; there may be but not generally)

Slide4:
_what are Delta_R, pT^track, pT^Jet? Please define.

Slide6:
pT,track should be consistent with as in slide4

Slide7:
If there are already approved preliminary, then mention "STAR
preliminary".

I probably missed it, Please point to me if these results were presented
before.

Cheers
Nihar

On 2022-10-17 00:47, webmaster--- via Star-hp-l wrote:
> Dear Star-hp-l AT lists.bnl.gov members,
>
> Tanmay Pani (tp543 AT physics.rutgers.edu) has submitted a material for a
> review, please have a look:
> https://drupal.star.bnl.gov/STAR/node/61350
>
> Deadline: 2022-10-27
> ---
> If you have any problems with the review process, please contact
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--

Sooraj Radhakrishnan

Research Scientist,

Department of Physics

Kent State University

Kent, OH 44243

Physicist Postdoctoral Affiliate

Nuclear Science Division
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road

Berkeley, CA 94720

Ph: 510-495-2473

Email: skradhakrishnan AT lbl.gov