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  • From: zli1 <zli1 AT rcf.rhic.bnl.gov>
  • To: Barbara Trzeciak <barbara.trzeciak AT gmail.com>
  • Cc: STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
  • Subject: Re: [Star-hp-l] HP-pwg meeting Thursday (11th May) 10 AM, BNL time
  • Date: Fri, 02 Jun 2023 00:28:31 +0800


Dear Barbara,

Thank you for your comments.

Indeed, we derive the yields from R_AA. This is because we directly combined R_AA from both channels beforehand, and as a result, deriving the yields from the combined R_AA was a straightforward method for us.

Regarding your concern about the treatment of uncertainties, these are handled using a simple error propagation principle, given that we are only multiplying R_AA by some constants. The systematic uncertainties include signal extraction, tracking, and particle identification (PID) uncertainties, and they do not incorporate any global uncertainties.

Best,
Ziyang

On 2023-06-01 18:57, Barbara Trzeciak wrote:
Hi Ziyang,

thanks for this update.
Regarding the inv. yields that you show on slide 13, why do you derive
the from RAA not directly from the corrected yields measured in Au+Au
in both channels ?
It looks like a way around. Though it's also fine, depending on how
you treat the uncertainties which I'm not sure about from the
statement "uncertainties based on RAA".
Could you please provide more details ?

Cheers,
Barbara

On Thu, Jun 1, 2023 at 10:44 AM zli1 via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:

Hi Nihar,

Thanks for your sign off, we may also want to upload those yields to

HPEData.

Best,
Ziyang
On 2023-06-01 15:17, Nihar Sahoo wrote:
Hello Ziyang,

Thank you for this explanation.

Do we have plan to publish also table in slide#13?

From my side, I sign off.

Cheers
Nihar


On 2023-06-01 11:16, zli1 wrote:
Hi Nihar,

Thanks for your question.

The issue you've noticed arises because the yield values of
dimuon
Y(2S) are negative in the mentioned bins (Cen010 and pT5_10). The
corresponding Y(2S) R_AA values from the dimuon channel are also
negative.

However, we didn't present these R_AA values (from either the
dimuon
or dielectron channel) in the slides or the paper. The R_AA
values
shown are the combined results, which are indeed positive.

I hope this clears up any confusion, and I'm happy to provide
further
explanation if needed.

Best,
Ziyang

On 2023-06-01 13:03, Nihar Sahoo wrote:
Hello Ziyang,

Thank you for updating these data tables.

Could you explain me (sorry for my ignorance) for dimuon Y(2s)
to
Y(1s) ratios and their stat. error are negative some cases, like
Cen010 and pT5_10, as in slide#5?
R_AA values are positive in those cases.

Cheers
Nihar


On 2023-06-01 08:21, zli1 via Star-hp-l wrote:
Hi All,

As we discussed before, I add values for the Y(1S), Y(2S),
Y(3S)
yields vs. centrality and vs. pt. And I also add the upper
limit for
Y(3S)/Y(1S) ratio. Please take a look at the revised slides in
below
link:

https://drupal.star.bnl.gov/STAR/system/files/Upsilon_ratio_0601.pdf

Would you kindly consider granting approval for uploading these

data?

Best,
Ziyang

On 2023-05-11 17:44, zli1 via Star-hp-l wrote:
Hi All,

Please find my slides in below link:
https://drupal.star.bnl.gov/STAR/system/files/2sto1sratio.pdf

Best,
Ziyang

On 2023-05-10 23:18, zli1 via Star-hp-l wrote:
Hi All,

I would like to present Upsilon(2S) to Upsilon(1S) ratio
based on
upsilon paper. I will send my slides later.

Best,
Ziyang

On 2023-05-08 21:55, Nihar Sahoo via Star-hp-l wrote:
Hello All,

We will have our HP-pwg meeting this Thursday (11th May) 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.

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,
Isaac, Yi, and Nihar
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Links:
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