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star-hp-l - Re: [Star-hp-l] HP-pwg meeting 10 AM BNL time, 10th Aug 2023

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Subject: STAR HardProbes PWG

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  • From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
  • To: Diptanil Roy <roydiptanil AT gmail.com>
  • Cc: STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>, Barbara Trzeciak <barbara.trzeciak AT gmail.com>, Yi Yang <yiyang0429 AT gmail.com>, "Mooney, Isaac" <isaac.mooney AT yale.edu>, Sevil Salur <sevil.salur AT gmail.com>
  • Subject: Re: [Star-hp-l] HP-pwg meeting 10 AM BNL time, 10th Aug 2023
  • Date: Thu, 17 Aug 2023 11:55:00 +0530

Hello Diptanil,

Thank you for your updates.
In addition to Rongrong's comment, Please find my additional comments below.

_Have you done any closure test for Z_jet^D correction procedure?

Slide21:
You have used now DCA < 3 cm, this may include some background tracks. Have you done any test with a strict DCA cut like 1, or 2 cm? Just to know if there is any effect with lesser background?
A bit concern for your Delta_R and Z results. Just to make sure there is no such contribution.

Slide4:
Can you please point to your raw distributions for Z_jet as well? Just to see how much the correction is?
Take one pT bin (say 1-10 GeV/c) for three centrality , and compare before and after correction.

Slide30:
1-10 GeV/c pT,D bins; central top plot; why systematic uncertainties are almost zero for intermediate p_T,jet^D0 bins, for example 8-12 GeV/c? Same for other plots.

Slide34:
1-10 GeV/c pT,D bin: R_cp central plot: do you understand why 0-0.2 bin has almost zero sys uncertainty?


Best
Nihar


On 2023-08-16 21:52, Diptanil Roy wrote:
Hi everyone, I have implemented the changes recommended yesterday in
the PWG meeting. Please find the updated presentation here.
https://drupal.star.bnl.gov/STAR/system/files/HardProbes_Aug10_Diptanil_v3.pdf

Here are some comments below:

1. Slide 11: I added the generated level input plots for PYTHIA+FONLL
distribution weighed by the data. They are shown in black.
2. Slides 27-38: I have added the new plots with the updates. Slide 26
summarises the updates. I have retained the old plots just in case you
wanted to compare them. For eg: Slide 27 has the jet pT spectra that I
showed yesterday. Slide 28 has the jet pT spectra after I moved the
central value to the mean of the prior variation.
3. Slides 39-44: I have the plots compared to available theory
predictions. I have added the prediction for peripheral events spectra
in D0 pT 1-10 GeV, and all the spectra in D0 pT 4-10 GeV.

Please let me know if you have any questions/comments.

Cheers,

On Tue, Aug 15, 2023 at 10:35 AM Diptanil Roy
<roydiptanil AT gmail.com> wrote:

Hi everyone, please find my contribution from today.

https://drupal.star.bnl.gov/STAR/system/files/HardProbes_Aug10_Diptanil_v2.pdf

Thank you for your comments.

Cheers,

On Tue, Aug 15, 2023 at 7:50 AM Barbara Trzeciak via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:

Thanks Jakub for the quick update.
Unfortunately, I won't be able to connect today for your
presentation.
Will check the discussion from the recording and let you know in
case of further questions.

Cheers,
Barbara

On Tue, Aug 15, 2023 at 1:09 PM Ceska, Jakub via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:

Dear Barbara,

thank you for your comments. Please find and updated version of the
presentation (same link,
https://drupal.star.bnl.gov/STAR/blog/ceskajak/HP-PWG-meeting-150823
[1]).

The pT bin fits (slides 24-29) are the first approach and can
definitely be improved. The 0-2 GeV/c bin would need a different
background shape, as the exponential does not work here). The plots
show a comparison of fits with Leszek's constraints (left) and with
larger, arbitrarily chosen constraints (right). Again, relaxing the
constraints improves the accuracy of the signal fit.

The constrained values used previously and the current values can
be found again on slides 22 and 23. The fit does not seem to succeed
for any unbound signal width and tends to grow to unexpectedly large
values of sigma. The upper constraint of 0.3 was chosen arbitrarily.


Best regards,
Jakub

-------------------------

Od: Barbara Trzeciak <barbara.trzeciak AT gmail.com>
Odesláno: úterý 15. srpna 2023 11:04
Komu: STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
Kopie: Ceska, Jakub <jakub.ceska AT fjfi.cvut.cz>
Předmět: Re: [Star-hp-l] HP-pwg meeting 10 AM BNL time, 10th Aug
2023

Hi Jakub,

thanks for the update. It looks like the peaks are wider. If it's
quick, can you do the same exercise for Upsilon signal divided in
Upsilon pT bins ?
It would be useful to add comparison of numerical values between
the previous constraint from Leszek fit parameters (mean and width)
and the ones that your new fit prefers.
And it would be good to see in more detail what happens with the
signal's width for J/psi in Brennan's analysis.

Cheers,
Barbara

On Tue, Aug 15, 2023 at 10:44 AM Ceska, Jakub via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:

Dear Barbara,

thank you for your comments. I have tried relaxing the widths (and
the means) of the CB functions. This appears to cover the signal
better. Please see slides 22 and 23 in the attached presentation:
https://drupal.star.bnl.gov/STAR/blog/ceskajak/HP-PWG-meeting-150823
[1]

As for the embedding, I am working on it, but have no results yet.

Best regards,
Jakub

-------------------------

Od: Barbara Trzeciak <barbara.trzeciak AT gmail.com>
Odesláno: pátek 11. srpna 2023 12:49
Komu: STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
Kopie: Ceska, Jakub <jakub.ceska AT fjfi.cvut.cz>
Předmět: Re: [Star-hp-l] HP-pwg meeting 10 AM BNL time, 10th Aug
2023

Hi Jakub,

thanks for the update on the fitting.
Looking at your slide 20, it seems that this left tail is part of
the signal. Could you please check what happens if you make looser
constraints to your Upsilon signal width.
Also, have you had a chance to look at the embedding to see if you
get such a wide signal there ?

Cheers,
Barbara

On Thu, Aug 10, 2023 at 2:11 PM Ceska, Jakub via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:

Dear all,

please find my slides attached:
https://drupal.star.bnl.gov/STAR/blog/ceskajak/HP-PWG-meeting-100823

Best,
Jakub

-------------------------

Od: Star-hp-l <star-hp-l-bounces AT lists.bnl.gov> za uživatele Ceska,
Jakub via Star-hp-l <star-hp-l AT lists.bnl.gov>
Odesláno: středa 9. srpna 2023 18:02
Komu: STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
Kopie: Ceska, Jakub <jakub.ceska AT fjfi.cvut.cz>
Předmět: Re: [Star-hp-l] HP-pwg meeting 10 AM BNL time, 10th Aug
2023

Dear all,

I will report on the questions raised last week and present an
update on the status of the analysis of the Run17 Upsilons.

If possible, I would like to present at the beginning of the
meeting, as I will need to leave by 12 EDT.

Best,
Jakub

-------------------------

From: Star-hp-l <star-hp-l-bounces AT lists.bnl.gov> on behalf of
张炜 via Star-hp-l <star-hp-l AT lists.bnl.gov>
Sent: Wednesday, August 9, 2023 3:47:06 PM
To: STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
Cc: 张炜 <wzhang AT m.scnu.edu.cn>
Subject: Re: [Star-hp-l] HP-pwg meeting 10 AM BNL time, 10th Aug
2023

Dear All,

I'd like to give an update on AuAu27、19.6、14.6GeV analysis.

Best,
Wei

------------------ Original ------------------

From: "STAR HardProbes PWG"<star-hp-l AT lists.bnl.gov>;
Date: Wed, Aug 9, 2023 07:53 PM
To: "STAR HardProbes PWG"<star-hp-l AT lists.bnl.gov>;
Cc: "Roy Chowdhury Priyanka
(DOKT)"<priyanka.roy_chowdhury.dokt AT pw.edu.pl>;
Subject: Re: [Star-hp-l] HP-pwg meeting 10 AM BNL time, 10th Aug
2023

Hello Nihar and all,

I will give an update on track merging issue for D0-hadron
femtoscopy. I will upload my slides later.

Regards,
Priyanka

-------------------------

From: Star-hp-l <star-hp-l-bounces AT lists.bnl.gov> on behalf of
Nihar Sahoo via Star-hp-l <star-hp-l AT lists.bnl.gov>
Sent: Tuesday, August 8, 2023 10:06 AM
To: Star-hp L <Star-hp-l AT lists.bnl.gov>
Cc: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
Subject: [Star-hp-l] HP-pwg meeting 10 AM BNL time, 10th Aug 2023

Hello All,

We will have our HP-pwg meeting this Thursday (10th Aug) at 10 AM
EDT.
Let us know please if you want to present and discuss your analysis
or
any other business.
Send your presentation slides a few hrs before the meeting, please.

As QM2023 deadline is approaching, we request all PAs to update us
your
status for your presentation/poster.

HP working group weekly meeting info:

https://drupal.star.bnl.gov/STAR/pwg/Hard-Probes/Weekly-HP-PWG-meeting

Join ZoomGov Meeting

https://bnl.zoomgov.com/j/1611419615?pwd=VW1hNm43ZDd5d2EvK2R4aEJsQ2ZNZz09
[2]

Meeting ID: 161 141 9615
Passcode: 744968

Regards,
Isaac, Yi and Nihar
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--

~ Neil

--

~ Neil

Links:
------
[1] https://drupal.star.bnl.gov/STAR/blog/ceskajak/HP-PWG-meeting-150823
[2] https://urldefense.com/v3/__https://bnl.zoomgov.com/j/1611419615?pwd=VW1hNm43ZDd5d2EvK2R4aEJsQ2ZNZz09__;!!P4SdNyxKAPE!C0kgtN_CyUdDd6WuslA8rEi7DLx1vclviJfToU_3a7peinSeePdJXpWZfWhg0YcbLANrvol1vGZ0UYrj4wv7tKrjRaP05bd6NUKv$




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