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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Egor Alpatov for ICPPA-2020 submitted for review

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: ShinIchi Esumi <esumi.shinichi.gn AT u.tsukuba.ac.jp>
  • To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Egor Alpatov for ICPPA-2020 submitted for review
  • Date: Sat, 26 Sep 2020 13:46:04 +0900

Dear Egoe
Thanks for the nice presentation of this new results. I have a few questions.

On p10, I would like to know why only some of the points does have quite
asymmetric systematic error?
And why for the most of your cases, the points are at the lower edge of the
systematic error? While on the
energy dependence comparison plots on the right panel, the previous data
points sit mostly on the opposite
edge of the systematic band...

The difference of the statistical errors between the two methods Xi and
Xi->Lambda would be mostly
coming from the alpha parameters, that is about a factor of two, where I do
see it for points at about 10-40%,
which is not really the case for the averaged points on the right panel, that
could be caused by the other effects
like the e.p. resolution etc… I just like to make sure how you average the
data for 20-50%, the inverse error
square weighing or number of particle and/or event weighting?

Since joey has also shown the centrality dependence of Lambda case in the
last QM, so I would like to have
a comparison to your left panel as well.
Best regards, ShinIchi

> On Sep 26, 2020, at 2:18, webmaster--- via Star-fcv-l
> <star-fcv-l AT lists.bnl.gov> wrote:
>
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Egor Alpatov (egroker1 AT gmail.com) has submitted a material for a review,
> please have a look:
> https://drupal.star.bnl.gov/STAR/node/52202
>
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov
> _______________________________________________
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