STAR Correlations and Fluctuations PWG

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

Dear Bijun,

Please find my comments on your nice poster:

Introduction:

Femtosopy, also known as HBT, -> Femtoscopy, baaed on HBT correlations for identical particles,

Please define: q_inv, r, \Psi(q_inv), S(r), Same(q_inv), Mixed(q_inv)

Then, define please \lambda, K_{coul}, R_{inv}

STAR Fixed target

n\sigmashift -> n\sigma shift (add a space)

& -> and

Summary:

At 3.0 ->At \sqrt{s_{NN}} = 3.0

With those implemented, I sign off. 

Enjoy the conferee!

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 EsumiShinIchi <esumi.shinichi.gn AT u.tsukuba.ac.jp> w dniu 30.08.2023, o godz. 02:40:

Dear Bijun

Thank you very much for the nice poster, as you know I have been 

assigned by Sooraj to review your poster for QM23 to help our very 

busy conveners, so I send you a few minor comments in the following. 

Best regards, ShinIchi

* I would spell out “Forward rapidity” for the both figures, in stead of “For-rapidity”. 

* In order not to confuse and to be consistent with upper panels, I would write 

  (repeat) “-1.0 < y < 0.5” in all the 4 panels, just like what you do in upper panel. 

* For the final plots with energy dependence, since the kinematic cuts are not 

  exactly same for all the beam energy, therefore I would add some additional 

  legend in the panel, like “0.4 < pT < 1.2 GeV/c"  "-0.5 < y < -0.3 ~ 0.0” for the 

  Mid-rapidity left panel, and “0.2 ~ 0.3 < pT < 1.2 GeV/c" "-1.0 < y < -0.5” for the 

  Forward rapidity right panel.

* I would also add some technical plots like "delta_phi* vs delta_eta” in the lower 

  left part of the poster, in order to indicate the close two-track resolution effects, 

  possibly with hole (two-track in-efficiency) and peak (ghost track) at (0,0). 

* I would choose to reverse the red and orange colors just for the right figure, in 

  order to have the merged track to be orange (or different color) and to make it 

  always red for the real track 1 and 2 just to make it consistent with the left figure. 

2023/08/30 1:53、樊碧君 via Star-cf-l <star-cf-l AT lists.bnl.gov>のメール:

Dear Hanna and Toshihiro, 

Sorry for the late submission of my poster and I have not received any comments yet.

If you are free, I am looking forward to your comments.

Thanks and regards, 

Bijun

 

 

------------------ Original ------------------

From:  "webmaster--- via Star-cf-l"<star-cf-l AT lists.bnl.gov>;

Date:  Mon, Aug 28, 2023 07:42 PM

To:  "star-cf-l"<star-cf-l AT lists.bnl.gov>;

Cc:  "webmaster"<webmaster AT star.bnl.gov>;

Subject:  [Star-cf-l] STAR presentation by Bijun Fan for Quark Matter 2023 submitted for review

 

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

Bijun Fan (bjfan AT mails.ccnu.edu.cn) has submitted a material for a review, 
please have a look:
https://drupal.star.bnl.gov/STAR/node/65004

Deadline: 2023-09-03
---
If you have any problems with the review process, please contact 
webmaster AT www.star.bnl.gov
_______________________________________________
Star-cf-l mailing list
Star-cf-l AT lists.bnl.gov
https://lists.bnl.gov/mailman/listinfo/star-cf-l

_______________________________________________
Star-cf-l mailing list
Star-cf-l AT lists.bnl.gov
https://lists.bnl.gov/mailman/listinfo/star-cf-l