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Subject: STAR Correlations and Fluctuations PWG

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From: Grigory Nigmatkulov <nigmatkulov AT gmail.com>
To: Wensong Cao <wensong814 AT mails.ccnu.edu.cn>, STAR Correlations and Fluctuations PWG <star-cf-l AT lists.bnl.gov>
Subject: Re: [Star-cf-l] [Note the US daylight time change] CF PWG meeting Nov. 10th (Thursday) 9:30am (BNL time)
Date: Thu, 10 Nov 2022 11:15:33 +0300

Hi Wensong,

Could you please plot the deta vs. dphi* distributions in the range from negative to positive values?

From the plots you show it is hard to see anything. What cuts have been used to construct these

angular correlations?

Another question is why do you think that the track-merging is removed by applying the cut?

Cheers,

Grigory

[Star-cf-l] [Note the US daylight time change] CF PWG meeting Nov. 10th (Thursday) 9:30am (BNL time), Xiaofeng Luo, 11/08/2022
- Re: [Star-cf-l] [Note the US daylight time change] CF PWG meeting Nov. 10th (Thursday) 9:30am (BNL time), Wensong Cao, 11/08/2022
- Re: [Star-cf-l] [Note the US daylight time change] CF PWG meeting Nov. 10th (Thursday) 9:30am (BNL time), Wensong Cao, 11/10/2022
  - Re: [Star-cf-l] [Note the US daylight time change] CF PWG meeting Nov. 10th (Thursday) 9:30am (BNL time), Grigory Nigmatkulov, 11/10/2022
    - Re: [Star-cf-l] [Note the US daylight time change] CF PWG meeting Nov. 10th (Thursday) 9:30am (BNL time), Wensong Cao, 11/10/2022