STAR Correlations and Fluctuations PWG

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

Dear Bijun,

Thank you for implementing my comments.

I sign off.

Kind regards,

Hanna

prof. dr hab. inż. Hanna Zbroszczyk
E-mail: hanna.zbroszczyk AT pw.edu.pl
Tel: +48 22 234 5851 (biuro)

Adres:
Poltechnika Warszawska

Wydział Fizyki
Zakład Fizyki Jądrowej
ul. Koszykowa 75
Biuro: 117b (via 115)
00-662 Warszawa

Wiadomość napisana przez Jun (via star-cf-l Mailing List) <star-cf-l AT lists.bnl.gov> w dniu 11.09.2024, o godz. 01:01:

Dear Hanna and all,

Thank you for your suggestions. I have implemented them and the new version can be found in the following link:

star.bnl.gov

As for Eq.3, cause our analysis is performed in PRF, what’s more, k*=1/2qinv for identical particles , so I prefer to remain it using f(k*).

Thank you!

Best regards,

Bijun

2024年9月9日 11:08，Hanna Zbroszczyk (via star-cf-l Mailing List) <star-cf-l AT lists.bnl.gov> 写道：

Dear Bijun,

Thanks for submitting your proceedings on time.

Please find below my comments:

Abstract, line 9, 10: R_G -> source size (as you should define the symbol first, so it is good enough just to mention in general source size)

Eq. 1: provide the formula for q_{inv} as q_{inv} = \sqrt{(p_1-p_2)^2 - (E_1-E_2)^2}.

Please note that q_{inv} is not defined in PRF, usually the quantities marked with asterisk are demoted in PRF, but  the wave function cannot contain them defined like this. As your analysis is not performed in PRF (as you use q_{inv} instead of k*), please make this equation proper in terms of quantities written in the formula (I assume you use LCMS but make sure about it looking in your code).

L24: N_{same}(q_{inv})) -> N_{same}(q_{inv})  - remove one ) and the same for N_{mixed}

Eq.2 : define R_G

Eq. 3: I am confused as you use k* here, you should rewrite this equations to be consistent with the reference frame you use in your analysis, make consistent and use q_{inv} where needed

L33: amplitude[3] -> amplitude [3]

L40: Kalman Filter(KF) -> Kalman Filter [3]

Figure 1: increase the figure or make the fonts larger (the should be at least of the size of the text of the proceedings)

L46: Afterburner)[6] -> Afterburner) [6]

L48: after K^0_S - K^0_S add „pairs"

L50: UrQMD plus CRAB -> UrQMD including CRAB to account for femtoscopic correlations

Figurę 2: increase the figure or the fonts on the figure

L59: results[7] -> results [7]

L81: remove: plus CRAB calculations

Thanks,

Hanna

Prof. Hanna Zbroszczyk, PhD, DSc, Eng.

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 Jun (via star-cf-l Mailing List) <star-cf-l AT lists.bnl.gov> w dniu 04.09.2024, o godz. 03:20:

Dear Nu and all,

Thank you for your patience. I have implemented them and upload the new version on the following link: https://drupal.star.bnl.gov/STAR/presentations/SQM-2024/Measurements-Kaon-Femtoscopy-AuAu-Collisions-sqrtsNN-30-45-GeV-STAR-Experim-1

Thank you!

Best regards,

Bijun

2024年9月2日 17:45，Nu Xu <nxu AT lbl.gov> 写道：

Hi Bijun and All,

1) Fig. 4 Caption: need to add a sentence at the end: “The dashed-line is the result of fitting pion <m_T>
dependence and the power-law parameter b =~ -0.3.  “

2) Line 40: need the reference for CRAB code;

3) In figures, we used “R_G” but in the texts we use “R_inv”. Let us use R_G so you do not have to change the figures;

4) In figures, we used “K_S^0 - K_S^0” but in the texts we use “K_S^0K_S^0”. Let us use K_S^0 - K_S^0 in texts so you do not have to change the figures;

Thank you,
Nu

On Sep 2, 2024, at 1:41 PM, 樊碧君 <bjfan AT mails.ccnu.edu.cn> wrote:

Dear Nu and all,

Thank you for your comments. I have implemented them and the new version can be found at the following link: https://drupal.star.bnl.gov/STAR/presentations/SQM-2024/Measurements-Kaon-Femtoscopy-AuAu-Collisions-sqrtsNN-30-45-GeV-STAR-Experim-1
I am not sure if I understand your comments correctly, if you have any further suggestions or comments, please let me know.

Thank you!
Best regards,
Bijun
 ------------------ Original ------------------
From:  "Nu Xu"<nxu AT lbl.gov>;
Date:  Mon, Sep 2, 2024 02:15 PM
To:  "star-cf-l"<star-cf-l AT lists.bnl.gov>;
Cc:  "nxu"<nxu AT lbl.gov>; "樊碧君"<bjfan AT mails.ccnu.edu.cn>;
Subject:  Re: [[Star-cf-l] ] Proceeding for SQM2024
Hi Bijun and All,

Thank you for the proceedings. My suggestions are marked in the pdf file.
Let u know in case you have questions.

Best regards,

Nu

On Sep 2, 2024, at 8:14 AM, 樊碧君 (via star-cf-l Mailing List) <star-cf-l AT lists.bnl.gov> wrote:

Dear Hanna, Nu, and all,

I have submitted a proceeding for the SQM2024, but seems like the "webmater AT star.bnl.gov" didn't have a response. Please kindly review the proceeding through the following link: https://drupal.star.bnl.gov/STAR/presentations/SQM-2024/Measurements-Kaon-Femtoscopy-AuAu-Collisions-sqrtsNN-30-45-GeV-STAR-Experim-1
Any comments or suggestions are welcome.

Thanks and regards,
Bijun