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Subject: STAR Flow, Chirality and Vorticity PWG
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[[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-fcv-l] ] STAR presentation by Aditya Rana for XXVI DAE-BRNS High Energy Ph... got commented by Subhash Singha
- Date: Sun, 15 Dec 2024 21:41:33 -0500
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
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