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Subject: STAR Flow, Chirality and Vorticity PWG
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Re: [[Star-fcv-l] ] STAR presentation by Aditya Rana for XXVI DAE-BRNS High Energy Ph... got commented by Subhash Singha
- From: subhash <subhash AT rcf.rhic.bnl.gov>
- To: star-fcv-l AT lists.bnl.gov
- Cc: aditya <aditya AT rcf.rhic.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: Mon, 16 Dec 2024 15:31:23 +0800
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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-
[[Star-fcv-l] ] STAR presentation by Aditya Rana for XXVI DAE-BRNS High Energy Ph... got commented by Subhash Singha,
webmaster, 12/15/2024
-
Re: [[Star-fcv-l] ] STAR presentation by Aditya Rana for XXVI DAE-BRNS High Energy Ph... got commented by Subhash Singha,
aditya, 12/16/2024
- Re: [[Star-fcv-l] ] STAR presentation by Aditya Rana for XXVI DAE-BRNS High Energy Ph... got commented by Subhash Singha, subhash, 12/16/2024
-
Re: [[Star-fcv-l] ] STAR presentation by Aditya Rana for XXVI DAE-BRNS High Energy Ph... got commented by Subhash Singha,
aditya, 12/16/2024
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