STAR Flow, Chirality and Vorticity PWG

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

Hello Everyone,
  If you are interested in studying isobar data please use the latest 
StRefMultCorr from Grigory. Please see the path below.
Best,
Prithwish


-------- Original Message --------
Subject: Re: [Star-cme-focusgroup-l] Notes-CME-fg meeting June 4, 2:30 
BNL time
Date: 2021-06-07 17:58
From: Grigory Nigmatkulov via Star-cme-focusgroup-l 
<star-cme-focusgroup-l AT lists.bnl.gov>
To: "Wang, Fuqiang" <fqwang AT purdue.edu>
Cc: Star-Cme-Focusgroup-L <star-cme-focusgroup-l AT lists.bnl.gov>
Reply-To: Grigory Nigmatkulov <nigmatkulov AT gmail.com>, 
star-cme-focusgroup-l AT lists.bnl.gov

Hi All,

We use (500, -0.5, 499.5) to estimate the centrality and fractions. For
the bins that are at the neighboring centralities
are placed, we splitted the bin integral (content) into 2 and added one
half to the bin on the right and one half
to the bin on the left. The bin center (integer value) will be the
refMultCorr cut.

The refMultCorr package have been updated and can be found here:

/star/u/gnigmat/soft/u/cme/StRoot/StRefMultCorr

The bin limits have also been checked and confirmed.

Cheers,

Grigory