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Subject: STAR Correlations and Fluctuations PWG
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Re: [Star-cf-l] Vz dependence of correlation function
- From: Grigory Nigmatkulov <nigmatkulov AT gmail.com>
- To: Wensong Cao <wensong814 AT mails.ccnu.edu.cn>
- Cc: STAR Correlations and FluctuationsPWG <star-cf-l AT lists.bnl.gov>
- Subject: Re: [Star-cf-l] Vz dependence of correlation function
- Date: Wed, 9 Nov 2022 13:17:27 +0300
Hi Wensong,
That is a very good study. Thank you very much for the plots. Indeed, for such a small Vz range it is hard to expect the difference.
My concern was about two-track cuts because of the mixing technique. Basically, tracks are emitted from different points because of the mixing
and one has to make sure that one compares tracks with identical initial parameters. Otherwise, two-track effects will be distorted.
Cheers,
Grigory
-
[Star-cf-l] Vz dependence of correlation function,
Wensong Cao, 11/01/2022
- Re: [Star-cf-l] Vz dependence of correlation function, Grigory Nigmatkulov, 11/09/2022
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