STAR Flow, Chirality and Vorticity PWG

[subhash <subhash AT rcf.rhic.bnl.gov>]

Dear Junyi,

Then I would suggest modifying the abstract (and title) including other 
FXT energies as well.

Thanks and regards,
Subhash

On 2024-12-18 01:41 PM, "Junyi Han" wrote:
> Dear Subhash,
>
> Thank you for your nice suggestions! I have update the abstract based
> on your suggestions, and it can be found in this link:
> https://drupal.star.bnl.gov/STAR/system/files/INPC_2025_abstract_v3.pdf.
>
> For hyper-nuclei v2, we don't make sure if we have enough statistics
> in other FXT energies to measure them. But for v1, I think we can
> include other FXT energies results. Thanks!
>
> Best regards,
> Junyi
>
> ------------------ Original ------------------
>
> From:  "webmaster"<webmaster AT star.bnl.gov>;
> Date:  Wed, Dec 18, 2024 03:16 AM
> To:  "STAR Flow, Chirality and Vortici"<star-fcv-l AT lists.bnl.gov>;
>
> Subject:  [[Star-fcv-l] ] STAR presentation by Junyi Han for INPC 2025
> got commented by Subhash Singha
>
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Subhash Singha ( connectsubhash AT gmail.com ) has commented on a
> material
> originally submitted by Junyi Han ( jyhan AT mails.ccnu.edu.cn ) at
> https://drupal.star.bnl.gov/STAR/presentations/INPC-2025/Flow-measurements-hyper-and-light-nuclei-AuAu-collisions-30-GeV-RHIC-1
>
> Comment:
> Dear Junyi, Nice abstract. I have following comments:
>
> l#7: About 2 billion minimum bias ....
> l#10: p, d, t, 3He and 4He
>
> Why do you want to focus on only 3 GeV, do you plan to include flow
> results
> from other FXT energies as well?
>
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