STAR Correlations and Fluctuations PWG

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

Dear Vinh,

Thank you very much for clarification. 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 Vinh Luong <lbavinh AT gmail.com> w dniu 31.10.2023, o godz. 14:27:

Dear Hanna,

Thank you very much for your comments and suggestions.

 

General comment: decide whether you mention all figures as: Fig. 1 or Figure 1

Linę 48: out-side-long -> „out-side-long”

Linę 55: remove a space after function,

Linę 58-59: out->„out, side->”side”, long-> „long”

Linę 60: out-long -> „out-long"

I have modified the proceedings accordingly.

 

Linę 23: 7.7 -> 13.7 

Here, I want to emphasize that RHIC can effectively work at 7.7 GeV as lowest, then energies lower than 7.7 GeV can be accessed only by FXT setup.

I have rephrased the sentence.

 

Figure 1, 2, 3, 4, 5- please increase the figure or increase the fonts.

I have set the maximum value for the figure's width and height as the journal's requirement. Also, I tried to increase the font size. Hope it looks better now.

 

References: line breaking does not work anywhere.

The double slash "//" is the citation format for this journal. 

Summary: (consider as Conclusion) please extend the physics discussion. Discuss more details, except of what was shown and that your results follow HADES and STAR observables. 

I have added physical discussions.

Please kindly have a look at the updated version: https://drupal.star.bnl.gov/STAR/system/files/ISHEPP_2023_PionFemto_STAR_FXT_Vinh_v2_0.pdf

Thank you and kind regards,

Vinh