STAR Correlations and Fluctuations PWG

[Hanna Paulina Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>]

Dear Moe,

Please find below my comments to your nice slides:

Slide 2: you have mentioned reference [1], but you refer to  [3], please change [3] -> [1] and write a full reference to PRL paper

Slide 3: add a reference to the femtoscopy technique

Slide 4: 2.8billion - 2.8 billion

Slide 5: add a reference to the KFParticle (if possible)

Descriptions on the plots are very small, is it possible to enlarge them? (axises, legends)

Slide 6: C_{true} is defined twice, please use another name

You have mentioned C_{measure} and C_{measured}, please describe better what you mean

Please explain the origin of the 2nd formula.

Please define Q_{inv}.

On slide 6 you mention „residual correlations” while on the slide 9 you mention feed-down correction.

Could you explain what do you mean by these two terms?

You have definition of q on the slide 3 and Q_{inv} on the slide 9 which are the same. Use just one term or compare them.

Slide 11: at 200 GeV -> ar \sqrt{s_{NN}} =  200 GeV

With those implemented, I sign off.

Thanks,

Hanna

Hanna Paulina Zbroszczyk

PhD DSc Eng, Professor WUT

E-mail: hanna.zbroszczyk AT pw.edu.pl

Tel: +48 22 234 5851 (office)

Address:

Warsaw University of Technology

Faculty of Physics

Nuclear Physics Division

Koszykowa 75

Office: 117b (via 115)

00-662 Warsaw, Poland

Wiadomość napisana przez webmaster--- via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 06.09.2021, o godz. 11:28:

Dear star-cf-l AT lists.bnl.gov members,

Moe Isshiki (k0nchar0127 AT gmail.com) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/56229

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