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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Rishabh Sharma for SQM 2022 submitted for review

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: subhash <subhash AT rcf.rhic.bnl.gov>
  • To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Cc: rishabhsharma AT students.iisertirupati.ac.in
  • Subject: Re: [Star-fcv-l] STAR presentation by Rishabh Sharma for SQM 2022 submitted for review
  • Date: Tue, 07 Jun 2022 18:34:44 +0800

Dear Rishabh,

Nice slides.
It was recommended by the management to release only 0-80% centrality results for 14.6 GeV. Please remove the corresponding v2 results in 0-30% and 30-80%.

slide#4: In the datasets, you can probably indicate BES-I and BES-II.

slide#5: Can you add comment on the improvement in EP resolution in BES-II compared to BES-I?

slide#6: Are these results from 0-80% or finer centrality bins? I would suggest to use 0-80%. Moreover, if you can replace these 14.6 GeV results with 19.6 GeV ones where the bad runs and centrality is finalized, it would be better. But I would leave it up to you.

slide#7: Can you add collision system, beam energy etc details inside these figures?

slide#8: Can you indicate the improvement in precision in BES-II relative to BES-I?

slide#9: Remove 14.6 0-30% and 30-80% plots. Mention centrality dependent study is underway.

slide#10: Can you use specific range of deviation, 10-20%?

slide#13: Indicate how much Deviation of light nuclei v2 scaling is observed.


Thanks and regards,
Subhash


On 2022-05-31 11:42 AM, webmaster--- via Star-fcv-l wrote:
Dear star-fcv-l AT lists.bnl.gov members,

Rishabh Sharma (rishabhsharma AT students.iisertirupati.ac.in) has submitted a
material for a review, please have a look:
https://drupal.star.bnl.gov/STAR/node/59779

---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
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