STAR Flow, Chirality and Vorticity PWG

[Prithwish Tribedy <ptribedy AT rcf.rhic.bnl.gov>]

Hi Ashik and all,
  During our isobar analysis we compiled a list of observables. This may 
give us some clue about which quantities are important:
https://drupal.star.bnl.gov/STAR/system/files/summary_qa_step2.html

I would still encourage people to provide input before Friday.
Best,
Prithwish


On 2021-10-17 12:36, ASHIK IKBAL via Star-fcv-l wrote:
> Hi FCV folks,
>
> We had a discussion on the QA variables for new and upcoming data sets
> in the last week QA board meeting. So far we (the QA team) are using
> the following variables for 19.6 GeV run-by-run QA analysis:
>
> 1       runidvsrefmult
>
> 2       runidvstofmatched
>
> 3       runidvsavgpt
>
> 4       runidvsavgeta
>
> 5       runidvsavgQ1x
>
> 6       runidvsavgQ1y
>
> 7       runidvsavgQ2x
>
> 8       runidvsavgQ2y
>
> 9       runidvsavgEpdQ1x
>
> 10      runidvsavgEpdQ1y
>
> 11      runidvsavgEpdQ2x
>
> 12      runidvsavgEpdQ2y
> 13.             runidvsbemcmatched
>
> The list of  badruns (identified based on the QA variables using
> automated run-by-run QA algorithm) is really necessary for the
> centrality team. The QA board has set a deadline of next Friday (Oct.
> 22) to finalize the variables.
>
> Please speak up if anyone wants to look at any other variables for the
> run-by-run QA analysis.
>
> Thanks,
> Ashik
>
> --
>
> Ashik Ikbal
>
> Research Associate
> Kent State University
> Department Of Physics
>
> Kent, OH 44242, USA
>
> Contact no.s: +1 631-504-7647 (USA)
>
>                       +91 8250216234 (India)
>
> Alternate e-mails: asheikh2 AT kent.edu
>                              ashik AT rcf.rhic.bnl.gov
>                              ashik.ikbal.sheikh AT cern.ch
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