STAR Flow, Chirality and Vorticity PWG

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

Dear Rishabh,

Nice proceedings. I have following suggestions for your consideration:

line 27: You could mention Beam Energy Scan in this line.
line 29: detectors.
line 31: allows the identification of ...
using a restriction on the mass-square (m2) of the particle.
line 32: It help improve particle ....
line 34: from
line 42: ... first order event plane determined by ...
line 44: remove "emitted in heavy-ion collisions"
line 61: "the mass number scaling within 20-30%." --> mention the pt/A 
range
line 63: as a function of rapidity (y) for ...
remove "measured"
line 64: Rephrase it to something like, Hyper-nuclei nuclei v1 results 
are compared with that of light nuclei ...
line 65-66: Linear fits are shown ... for other light nuclei species" 
--> rephrase this line.
line 75: that coalescence could be the dominant mechanism for 
hyper-nuclei
line 78 and 82: mention the beam energies

For figures: You could mention statistical and systematic uncertainties 
in captions.

I sign off once these are addressed.

Thanks and regards,
Subhash

On 2022-08-19 02:46 PM, 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/60567
>
> Deadline: 2022-08-28
> ---
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