STAR Correlations and Fluctuations PWG

[Kincses Dániel <kincses AT ttk.elte.hu>]

Dear Xiaofeng,

Thank you, I implemented the changes!

Cheers,
Daniel

---

Feladó: Star-cf-l <star-cf-l-bounces AT lists.bnl.gov>, meghatalmazó: Xiaofeng Luo via Star-cf-l <star-cf-l AT lists.bnl.gov>
Elküldve: 2022. július 10., vasárnap 3:54
Címzett: Kincses Dániel via Star-cf-l <star-cf-l AT lists.bnl.gov>
Tárgy: Re: [Star-cf-l] STAR presentation by Daniel Kincses for WPCF 2022 submitted for review

 

Hi Daniel,

     Nice presentation.
     I only have minor suggestion:
     1. Slide 13, Right plot, legend of mT range, please use : 0.7<mT<0.78
     2. Slide 16, The plotting style of dashed line of Guassian
distribution looks like a continuous solid line. Please change it.

     With those implemented, I sign off.

Thank you,
Best Regards,
Xiaofeng

On 2022/7/10 02:52, Kincses Dániel via Star-cf-l wrote:
> Dear Hanna,
>
> Thank you for the feedback! I uploaded the revised version
> (https://drupal.star.bnl.gov/STAR/presentations/WPCF-2022/Bose-Einstein-correlations-charged-kaons-produced-sqrtsNN-200-GeV-AuAu-col-3) and
> here are my answers:
>
> Slide 1: Please put the logo of U.S. department of Energy at some
> other place at the slide and add „Partially funded by …" --> done
> Slide 3: Define \Psi(x_1, x_2) function --> done
> It would be nice to have written that it includes QS effects and FSI
> --> done
> Slide 4: Define \alpha(K), R(K); here you use q, on the previous slide
> you use Q, please make them consistent
> --> I deleted the K dependence from the top line, and added a comment
> about it at the end of the slide
> --> the q on slide 4 is different from Q on slide 3, the Levy-stable
> distribution is defined with a Fourier-transform
> Slide 10: do you have dE/dx plot just for accepted kaons? --> included
> Slide 11: please confirm whether FMH<0.001 or FMH < 0.01 or FMH < 0.1
> --> It is FMH < 0.001, essentially only accepting FMH = 0 or FMH = -1
> Define \delta z and \delta u --> done
> Slide 13: define k_T --> done
> Could you please add also result of the Gaussian fit (for a comparison
> with Levy) --> We only have preliminary for this example fit, do not
> have it for a Gaussian (fixed alpha = 2)
> Slide 14: define N_C and N_H --> done
> Comment to slide 14 and 15: it would be nice to have here results of
> \lambda and R for Gaussian fit, and to compare those with pions
> results. --> Again, we do not have preliminary for such plots
> unfortunately, nor I have them ready to show; Later at a PWG meeting
> we could present such plots if needed.
>
> Thanks a lot,
> Daniel
> ------------------------------------------------------------------------
> *Feladó:* Star-cf-l <star-cf-l-bounces AT lists.bnl.gov>, meghatalmazó:
> Hanna Paulina Zbroszczyk via Star-cf-l <star-cf-l AT lists.bnl.gov>
> *Elküldve:* 2022. július 8., péntek 22:05
> *Címzett:* star-cf-l AT lists.bnl.gov <star-cf-l AT lists.bnl.gov>
> *Tárgy:* Re: [Star-cf-l] STAR presentation by Daniel Kincses for WPCF
> 2022 submitted for review
> Hi Daniel,
>
> Please find my comments to your nice slides below:
>
> Slide 1: Please put the logo of U.S. department of Energy at some
> other place at the slide and add „Partially funded by …"
> Slide 3: Define \Psi(x_1, x_2) function
> It would be nice to have written that it includes QS effects and FSI
> Slide 4: Define \alpha(K), R(K); here you use q, on the previous slide
> you use Q, please make them consistent
> Slide 10: do you have dE/dx plot just for accepted kaons?
> Slide 11: please confirm whether FMH<0.001 or FMH < 0.01 or FMH < 0.1
> Define \delta z and \delta u
> Slide 13: define k_T
> Could you please add also result of the Gaussian fit (for a comparison
> with Levy)
> Slide 14: define N_C and N_H
> Comment to slide 14 and 15: it would be nice to have here results of
> \lambda and R for Gaussian fit, and to compare those with pions results.
>
> With those implemented, 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 Hanna Paulina Zbroszczyk
>> <hanna.zbroszczyk AT pw.edu.pl> w dniu 08.07.2022, o godz. 21:38:
>>
>> Hi Daniel,
>>
>> For some reason I am unable to delete multiple entries.
>> I will pick one of them and will comment soon.
>>
>> 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 Kincses Dániel via Star-cf-l
>>> <star-cf-l AT lists.bnl.gov> w dniu 04.07.2022, o godz. 13:10:
>>>
>>> Dear All,
>>>
>>> Sorry for accidentally uploading multiple entries, I had some
>>> connection issues.
>>>
>>> Cheers,
>>> Daniel
>>> ------------------------------------------------------------------------
>>> *Feladó:*Star-cf-l <star-cf-l-bounces AT lists.bnl.gov>, meghatalmazó:
>>> webmaster--- via Star-cf-l <star-cf-l AT lists.bnl.gov>
>>> *Elküldve:*2022. július 4., hétfő 12:42
>>> *Címzett:*star-cf-l AT lists.bnl.gov<star-cf-l AT lists.bnl.gov>
>>> *Tárgy:*[Star-cf-l] STAR presentation by Daniel Kincses for WPCF
>>> 2022 submitted for review
>>> Dear star-cf-l AT lists.bnl.gov members,
>>>
>>> Daniel Kincses (kincses AT ttk.elte.hu) has submitted a material for a
>>> review,
>>> please have a look:
>>> https://drupal.star.bnl.gov/STAR/node/60162
>>>
>>> ---
>>> If you have any problems with the review process, please contact
>>> webmaster AT www.star.bnl.gov
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>>
>
>
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--
Xiaofeng Luo
Professor of Physics
College of Physical Science and Technology
Central China Normal University
Luoyu Road 152, Wuhan China
Office Phone #: +86-27-67867500

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