Skip to Content.
Sympa Menu

star-cf-l - Re: [Star-cf-l] Preliminary Plots

star-cf-l AT lists.bnl.gov

Subject: STAR Correlations and Fluctuations PWG

List archive

Chronological Thread  
  • From: Nu Xu <nxu AT lbl.gov>
  • To: Rutik Manikandhan <manikandhan.rutik AT gmail.com>
  • Cc: Nu Xu <nxu AT lbl.gov>, Hanna Paulina Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>, STAR Correlations and Fluctuations PWG <star-cf-l AT lists.bnl.gov>
  • Subject: Re: [Star-cf-l] Preliminary Plots
  • Date: Mon, 29 Jan 2024 10:55:49 -0800

Hi Rutik and All,

Here are my suggestions regarding to the three plots:
1) Plot 1: It is difficult to seperate statistical from systematic
uncertainty. Let us try to use a light-yellow band to represent the
systematic uncertainty;
2) Plot 2: add “STAR Preliminary” to the figure. This figure always confuses
me: what is the width of the peso-rapidity bin used in Plot 1? What is the
purpose to show this plot outside STAR experiment?
3) Plot 3: add “STAR Preliminary” to the figure. add “3 GeV Au+Au Collisions”
to the plot.
What do we learn from this figure? What is the width of the peso-rapidity
bin used in Plot 1?

Please update these plots. If you have time, we can discuss over zoom. I will
have other meetings soon. But we can discuss at about 3pm PT.

Best regards,
Nu

> On Jan 29, 2024, at 10:02 AM, Rutik Manikandhan
> <manikandhan.rutik AT gmail.com> wrote:
>
> Hello Conveners,
>
> Here are the plots for the preliminary request from last week.
> Do let me know of any changes that need to be made.
> https://drupal.star.bnl.gov/STAR/system/files/Preliminary_Plots.pdf
>
> Best,
> Rutik Manikandhan
> PhD Candidate, Experimental High Energy Group
> Physics Dept.
> University of Houston





Archive powered by MHonArc 2.6.24.

Top of Page