STAR Flow, Chirality and Vorticity PWG

[Nu Xu <nxu AT lbl.gov>]

Hi Subhash,

I would suggest we stay with 3GeV for the time being as the statistics is the 
best from the energy. It is important for hyper-nuclei results on 
collectivity.
For example, the statistics will be very poor for v2 measurements of 
hyper-nuclei.

Thanks,
Nu

> On Dec 17, 2024, at 10:28 PM, subhash <subhash AT rcf.rhic.bnl.gov> wrote:
> 
> 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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