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star-cf-l - Re: [Star-cf-l] STAR presentation by Yu Zeng for Quark Matter 2023 submitted for review

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Subject: STAR Correlations and Fluctuations PWG

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  • From: "曾钰" <zengy AT mails.ccnu.edu.cn>
  • To: "star-cf-l" <star-cf-l AT lists.bnl.gov>
  • Subject: Re: [Star-cf-l] STAR presentation by Yu Zeng for Quark Matter 2023 submitted for review
  • Date: Mon, 28 Aug 2023 20:57:53 +0800

Dear Hanna and Toshihiro,
Thanks very much for you comments. I have implemented them and reupload my poster.
Please have a look: https://drupal.star.bnl.gov/STAR/system/files/Yu_Zeng_QM2023_poster_v2_.pdf
Cheers,
Yu Zeng

 
 
------------------ Original ------------------
From:  "野中俊宏 via Star-cf-l"<star-cf-l AT lists.bnl.gov>;
Date:  Sat, Aug 26, 2023 09:44 PM
To:  "star-cf-l"<star-cf-l AT lists.bnl.gov>;
Cc:  "nonaka.toshihiro.ge"<nonaka.toshihiro.ge AT u.tsukuba.ac.jp>;
Subject:  Re: [Star-cf-l] STAR presentation by Yu Zeng for Quark Matter 2023 submitted for review
 
Dear Yu,

I have a few minor suggestions on your nice poster presentation.

- Section title “Correlation Function” -> “Correlation function”, “Results and Summary” -> “Results and summary”

- Make axis labels/titles and legends bigger.

- (Summary) The centrality and rapidity dependence…

With these implemented, I sign off.

Best regards,
Toshihiro

差出人: Star-cf-l <star-cf-l-bounces AT lists.bnl.gov> が Hanna Paulina Zbroszczyk via Star-cf-l <star-cf-l AT lists.bnl.gov> の代理で送信
送信日時: 2023年8月26日 21:50
宛先: star-cf-l AT lists.bnl.gov <star-cf-l AT lists.bnl.gov>
CC: Hanna Paulina Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>
件名: Re: [Star-cf-l] STAR presentation by Yu Zeng for Quark Matter 2023 submitted for review
 
Dear Yu,

Please find below my comments on your nice poster.

Add a space between your name and email and the comma after your email.

Abstract: I suggest not mentioning QGP as at 3.2 GeV, we don’t expect it.
Will be shown -> are shown

Femtoscopy section: Two-particle -> two-particle
function(referred -> function (referred
spacetime -> space-time
and Twiss interferometry -> and Twiss interferometry [1] (add a reference)

I suggest here to mention not only the fact that in astronomy, the properties of stars are determined but also that we deal with different orders of size magnitudes (HIC: fm, astronomy: tens of m), and that in astronomy, the signal intensities are measured, while in HIC the momenta of emitted particles (to extend little bit what is seen on the figure).
Please add the reference to the figure.

Correlation Function:
Define N, P(p-1, p_2), P(p_1), P(p_2), S(r)

Track-splitting effect:
two(Track1 and Track2) -> two (track 1, track 2)

Track-merge effect:
tracks(Track1 and Track2) -> tracks (track 1 and track 2)

Results and Summary,
Please increase the font sizes at your figures (axis, scales)
Source size is extracted -> Extract the source size
You can mention f_0 and d_0 parameters when you write the effective range and the scattering length.
You can add [3] reference here.

Add a place where you mention [2] reference.

With those implemented, I sign off.

Enjoy the conference,

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 25.08.2023, o godz. 18:15:

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

Yu Zeng ( zengy AT mails.ccnu.edu.cn) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/64886

Deadline: 2023-09-03
---
If you have any problems with the review process, please contact  
webmaster AT www.star.bnl.gov
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