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star-hp-l - Re: [Star-hp-l] HP-pwg meeting Thursday (6th Oct) 10 AM, BNL time

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  • From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
  • To: Tristan Protzman <tlp220 AT lehigh.edu>, STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
  • Subject: Re: [Star-hp-l] HP-pwg meeting Thursday (6th Oct) 10 AM, BNL time
  • Date: Fri, 07 Oct 2022 18:51:53 +0530

Hi Tristan,

Great, it looks good.

Two suggestions on your results.

1) If I look at your Slide#14 jet v2 plot, the systematic uncertainty bands for 1st and 3rd bins are relatively tiny compared to other bins. Generally systematic uncertainty should show a continuous variation throughout the bins. Hence I suggest to use the 2nd bin's sys uncertainty for 1st bin and average value of 2nd and 4th's sys uncertainty for 3rd bins. For future we can discuss and work on it.
Same for the plot in slide#15.

2) SLide#14 and 15 płot, Please include inside each figure "No jet pT-correction applied".

if I find more comment and suggestion, I will let you know.

Remaining comments inline.

On 2022-10-07 05:31, Tristan Protzman via Star-hp-l wrote:
Hi all,

I have updated my preliminary figure request slides with the feedback
I received this morning: Preliminary Figure Request: Azimuthal
Anisotropy of Jets in √(s_NN )=200 GeV Ru+Ru and Zr+Zr Collisions
(bnl.gov) [2]

Most notably, I verified the behavior of the toy model for both zero
and non-zero flow. Using the hard core framework, the appropriate
values are recovered. This is shown on slide 22.

THis is a very nice study on two extreme cases for jet v2 values.
But there is one point I want to make here (that I forgot to discuss yesterday's meeting) that we need to check this study when you increase for jet R > 0.2; probably this we can discuss after HQ.


I have also used the variation of the background modulation as the
dominant systematic uncertainty, shown on the updated main figure
(slide 14). Details of this are on slide 23, but they are determined
by the average change in a point's value by varying the background
modulation by +- 0.02.

this is good.

The jobs to study the effects of throwing out
4% of tracks are submitted, but have been sitting idle in the queue
all day unfortunately.

Let us know when you finish this and update all your sys. uncertainties.


Cheers
Nihar
Cheers,
Tristan

On Thu, Oct 6, 2022 at 1:10 PM Yi Yang via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:

Thanks a lot, Rachael!

Cheers,
Yi

On Thu, Oct 6, 2022 at 11:54 PM Rachael Botsford <rab420 AT lehigh.edu>
wrote:

https://drupal.star.bnl.gov/STAR/blog/rbotsford/DNP-2022-First-Draft

On Thu, Oct 6, 2022 at 10:21 AM Yi Yang <yiyang0429 AT gmail.com>
wrote:

Hi Rachael,

Could you please put your slides to the drupal and send the link to
us? Thanks a lot.

Cheers,
Yi

On Wed, Oct 5, 2022 at 2:58 AM Rachael Botsford via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:

Hi,
I would like to present a draft of my talk for the DNP.
Thanks,
Rachael

On Tue, Oct 4, 2022 at 12:30 PM Nihar Sahoo via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:
Hello HP folks,

We will have our regular HP-pwg meeting this Thursday (6th Oct) at
10
AM BNL time. Let us know if you want to present or update your
analysis.

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
[1]

Meeting ID: 161 141 9615
Passcode: 744968

Regards,
Barbara, Yi, Sooraj, and Nihar
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Links:
------
[1] https://urldefense.com/v3/__https://bnl.zoomgov.com/j/1611419615?pwd=VW1hNm43ZDd5d2EvK2R4aEJsQ2ZNZz09__;!!P4SdNyxKAPE!HylmnhXcg9VzfW6H5-cJTUOu4aGoaxl4stGbsUHSGTZ5dxAHVgHFXKeYLGTmyspPcDnp_OBtQQIroEFW3fJImSKZ$
[2] https://drupal.star.bnl.gov/STAR/system/files/Protzman_JetV2_%20Preliminary_Figure_Request_v4.pdf
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