STAR Correlations and Fluctuations PWG

[Dylan Neff <dneffucla AT gmail.com>]

Hi Hanna,

Thanks very much for the comments! I've tried to implement your suggestions as best I could and have uploaded the new slides, please let me know if you have further suggestions.

https://drupal.star.bnl.gov/STAR/node/56613

It was also pointed out to me that two of the plots don't contain STAR data (just AMPT) so don't need the preliminary label. I've updated the preliminaries page as well.

Thanks,

Dylan Neff

On Fri, Oct 1, 2021 at 5:59 AM Hanna Paulina Zbroszczyk via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:

Dear Dylan,

Slide 3: add please here more motivation’s description to explain better why you use these different divisions.

Explain what you gain with this method. Why one should expect different distributions in different divisions?

Slide 8: what is the physics conclusion from these plots? Add it to the slide.

Slide 10: similarly, please add the physics message provided with these plots.

Slide 13: Add a physics interpretation to the summary too.

General comment to the slides: 8, 10, 11, 12:

As we discussed yesterday, please refresh your preliminary plots adding more descriptions to the legends of the figures.

When ready, please create an entry at our data base of preliminary plots (you can find the link at the main page of our meeting and in the email we send before each meeting too)

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 29.09.2021, o godz. 23:07:

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

Dylan Neff (dneff AT physics.ucla.edu) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/56613

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