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star-fcv-l - Re: [[Star-fcv-l] ] STAR presentation by Aditya Rana for XXVI DAE-BRNS High Energy Ph... got commented by Subhash Singha

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: aditya <aditya AT rcf.rhic.bnl.gov>
  • To: star-fcv-l AT lists.bnl.gov
  • Subject: Re: [[Star-fcv-l] ] STAR presentation by Aditya Rana for XXVI DAE-BRNS High Energy Ph... got commented by Subhash Singha
  • Date: Tue, 17 Dec 2024 09:45:22 +0530

Dear Subhash,

Thank you for your suggestions and pushing the presentation to star-talk.

I have implemented your suggestions and updated the slides.

Thanks and regards
Aditya

On 2024-12-17 04:40, subhash wrote:
Dear Aditya,

I think it is bit odd to show points with zero systematic error for
peripheral bins. In this case, since you don't have much time left
before the conference we suggest removing the peripheral bins on
slide#11, 12. This wouldn't cause any change in your physics
conclusion.
With this suggestion, I am pushing it to star-talks.

Thanks and regards,
Subhash

On 2024-12-16 06:25 PM, aditya wrote:
Dear Subhash,

I have attached plot to show systematic variation for covariance of v3
and A for both Ru+Ru and Zr+Zr. In the plot it can be seen that for
the last centrality bin, statistical errors are large as compared to
the rest of the centrality bins and by using Barlow check systematics
comes out to be zero.

Hope this clears the doubt. If there are any further suggestions and
questions please let me know.

Regards,
Aditya

On 2024-12-16 13:01, subhash wrote:
Dear Aditya,

Thanks for your answer. I have one follow up comment:

s#11: I see that you apply Barlow check. But having zero systematic
seems odd, because rest of bins or neighboring bins have large
systematic, comparable to your statistical errors. Please check if you
can improve for those points. Also, do you have a plot to show
systematic variations?

Thanks and regards,
Subhash


On 2024-12-16 03:13 PM, aditya wrote:
Dear Subhash,

Thank you for your comments and suggestions.

Below are the answers for your queries:

s#4: Why do you have the same number of events, isn't that Zr+Zr has
more than Ru+Ru?
These are number of events after cut. I have now mentioned this on this slide.

s#10: you could spell out RFP and POI, for the first time either here
or in previous slides?
I have added this on this slide now.


s#11: Why is the systematic error smaller for most peripheral bins?
I used Barlow Check to calculate the Systematic uncertainties. The statistical errors are large for peripheral bins, these large fluctuations overshadow systematic variation and thus results in small or no systematic errors by Barlow Check.

s#12: Are these errors on the plot statistical or both syst and stat
combined, please mention it.
I have included the systematic error bars now to the plot, were not included before.

I have updated the presentation. Please let me know if further changes
are required.

Presentation is available at following link,
https://drupal.star.bnl.gov/STAR/node/70221

Thanks and regards
Aditya

On 2024-12-16 08:11, webmaster AT star.bnl.gov wrote:
Dear star-fcv-l AT lists.bnl.gov members,

Subhash Singha ( connectsubhash AT gmail.com ) has commented on a material
originally submitted by Aditya Rana ( aditya.rna2 AT gmail.com ) at
https://drupal.star.bnl.gov/STAR/presentations/XXVI-DAE-BRNS-High-Energy-Physics-Symposium-2024/Probing-Chiral-Magnetic-Wave-isobar-0

Comment:
Nice slides. I have a few questions and  suggestions:
s#4: Why do you have the same number of events, isn't that Zr+Zr has more
than Ru+Ru?
s#10: you could spell out RFP and POI, for the first time either here or in
previous slides?
s#11: Why is the systematic error smaller for most peripheral bins?
s#12: Are these errors on the plot statistical or both syst and stat
combined, please mention it.

I sign off with these addressed.

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