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star-fcv-l - Re: [Star-fcv-l] Special FCV meeting on Tuesday March 15, 9:30 am EST.

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: ShinIchi Esumi <esumi.shinichi.gn AT u.tsukuba.ac.jp>
  • To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] Special FCV meeting on Tuesday March 15, 9:30 am EST.
  • Date: Wed, 16 Mar 2022 18:50:08 +0900

Dear Rishabh
I’m questioning the same thing to everyone yesterday in the special pwg
session,
it looks like you also have the similar problem in your re-centering
calibration, as we
still see about a half of the 1st moment of the non-flatness even after the
re-centering
calibration in your page 8, which tells me there is some problem in the
method. You
could look at the Priyanshi’s slide page 7, where we only see the higher
order contributions
than 1st order moments in a remaining non-flatness after the re-centering
calibration,
that is what is supposed to be, although the formula in the page 6 has some
issues.
So please make sure your re-centering correction is OK or not. It is flat
after the final
Fourier shift correction, so that the final results might still be OK, but it
would be better
to do it right. In stead of re-centering the q-vector, which should be done
in event-wise,
one can do an inverse weighting factor correction (track-wise) with measured
azimuthal
distribution. You can go back to the famous "flow bible" from Sergei and Art
in '96.
Best regards, ShinIchi

> 2022/03/14 3:16、subhash via Star-fcv-l <star-fcv-l AT lists.bnl.gov>のメール:
>
> Dear All,
>
> We will hold an additional FCV meeting this Tuesday, March 15, at 9:30 am
> EST. This is a special meeting to accommodate some QM talk/posters for
> which we have not received the request for preliminary. We would request
> you to make a short presentation following:
> https://drupal.star.bnl.gov/STAR/system/files/Prelim_Request_template.pdf
>
> Since the QM is in a few weeks from now, it will be too late for us to
> review and sign off your analysis if you can't present. Thanks for your
> understanding.
>
> Best regards,
> Jiangyong, Prithwish and Subhash
>
>
> The tentative agenda can be found below:
> https://drupal.star.bnl.gov/STAR/blog/jjiastar/bulkcorr
>
> (Special Meeting for QM-approval) March 15, 2022:
> 1. Joey Adams -- lambda polarization
> 2. Gavin Wilks -- phi spin alignment
> 3. Shuai Zhou -- PID v2 BES
> 4. Diyu Shen -- charge dependent v1
> 5. Aditya Prasad -- charge dependent v1
> 6. Eddie Duckworth -- net proton v1
> 7. Niseem Magdy -- flow momentum correlation
>
> We shall use the FCV zoom link:
> https://urldefense.com/v3/__https://stonybrook.zoom.us/j/95735410810?pwd=M2JRZDBDSng4MG5SYmx6dlppYXhLZz09__;!!P4SdNyxKAPE!UXhP_DS8ys-TdWPw0_Vm4ATdCQdbWUfil5xQC2X14Niv1NnkB5575iHyZ29jG4Z4AVeuU8wc$
>
> Meeting ID: 957 3541 0810
> Passcode: 486227
>
>
> _______________________________________________
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> Star-fcv-l AT lists.bnl.gov
> https://lists.bnl.gov/mailman/listinfo/star-fcv-l





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