STAR Correlations and Fluctuations PWG

[Xiaofeng Luo <xfluo.star AT hotmail.com>]

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