STAR task force for evaluating tracking efficiency uncertainty

[Petr Chaloupka <petrchal AT rcf.rhic.bnl.gov>]

Hello Robert,

thanks a lot. The DCA worries me a bit. Let's discuss tomorrow.

With best regards,
Petr

On 12. 06. 23 17:15, Robert Líčeník wrote:

Hi Petr, Yuri,

I added the requested plots to the slides (at the end):

https://drupal.star.bnl.gov/STAR/system/files/TrackingEffTask_061223_v2_0.pdf

We can discuss tomorrow,

Robert

On Mon, Jun 12, 2023 at 4:26 PM Fisyak, Yuri V <fisyak AT bnl.gov> wrote:

Hi Robert, thank you for plots.

  I see two main differences in kinematics:

<pT>_MC ~ 2 <pT>_RC, and Phi_MC is more flat than Phi_RC,

But these differences cannot explain difference in efficiency.

Can your provide two more plots:

2D: NoFitpL versus NoFitpK for RC and MC, and Match Chisq

?

                                                              Yuri Fisyak

STAR                                           Phone: +1 631 344 3913
Brookhaven National Laboratory  Fax:    +1 631 344 4206
510A/1-161
http://www.star.bnl.gov/~fisyak       E-mail: fisyak AT bnl.gov

 

 

 

From: Star-tf-trkeff-l <star-tf-trkeff-l-bounces AT lists.bnl.gov> on behalf of Robert Líčeník via Star-tf-trkeff-l <star-tf-trkeff-l AT lists.bnl.gov>
Date: Monday, June 12, 2023 at 9:35 AM
To: Petr Chaloupka <petrchal AT rcf.rhic.bnl.gov>
Cc: STAR task force for evaluating tracking efficiency uncertainty <star-tf-trkeff-l AT lists.bnl.gov>
Subject: Re: [Star-tf-trkeff-l] Tracking Efficiency Uncertainty meeting June 6, 2023, 10:00 AM

Hello everyone, 

 

I have updated the slides (beginning with slide 12) and you can see the distributions for positive tracks only.

https://drupal.star.bnl.gov/STAR/system/files/TrackingEffTask_061223.pdf

I still see very much different tracking efficiency.

 

Thanks,
Robert

 

On Mon, Jun 12, 2023 at 10:36 AM Robert Líčeník <licenik AT ujf.cas.cz> wrote:

Hi Yuri and Peter,

 

thanks for pointing that out. I am a little surprised to see such a significant effect of the track charge on the efficiency.

Is this the correct way to select only positively charged tracks:

pTi > 0 for K tracks and pTi < 0 for L tracks?

It seems like in the simulation plots we also see some tracks which correspond to negative charge, so I just want to make sure that this is the way to go.

 

Thanks,
Robert

 

On Sat, Jun 10, 2023 at 11:20 PM Petr Chaloupka <petrchal AT rcf.rhic.bnl.gov> wrote:

Hello Robert,

thanks a lot for making the. As Yuri pointed out I only simulated positive poins. Could you try to cut on the charge in both data and simulation?

With best regards,
Petr

On 09. 06. 23 14:46, Robert Líčeník wrote:

Hi everyone,

 

as discussed during the meeting, I have put together a few slides comparing results from cosmics data and simulation.

Please let me know if you have any suggestions or if you would like to see some additional plots.

The slides are uploaded at the meeting link below:

https://drupal.star.bnl.gov/STAR/event/2023/06/06/Tracking-Efficiency-Uncertainty-meeting/Cosmics-update

 

Thanks,
Robert

 

 

On Mon, Jun 5, 2023 at 9:44 PM Petr Chaloupka via Star-tf-trkeff-l <star-tf-trkeff-l AT lists.bnl.gov> wrote:

Dear All,

Please join our meeting tomorrow at 10:00 New York time.
Please upload any material for discussion to the drupal page:
https://drupal.star.bnl.gov/STAR/event/2023/06/06/Tracking-Efficiency-Uncertainty-meeting


With best regards,
Petr


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