STAR Flow, Chirality and Vorticity PWG

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

Dear Jie,

Nice presentation. I have a few comments for your consideration:

s#6: For general audience, it might be good to indicate the invariant 
mass distribution is after mixed-event subtraction.
Are their any constraint used for f0, f2 and rho, I mean do you keep 
mass, width for all of them as free, or constrain them in some way? How 
do you constrain the blue line? Looks like the blue line do not explain 
the background shape. Do you have systematic error due to different 
background shapes along with varying normalization scales? This must 
have been discussed, but I might have missed those.

s#7: It is not clear which function you use for mass and width 
extraction, rel. BW or simple BW?

s#15: Correct typo: "scaling"
An error projection figure for f0 v2 and a projected n_q value would be 
nice, but it is up to you.

Thanks and regards,
Subhash



On 2022-08-29 11:20 AM, webmaster--- via Star-fcv-l wrote:
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