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star-cf-l - [Star-cf-l] Run19 19.6 GeV centrality definition available in StRefMultCorr

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Subject: STAR Correlations and Fluctuations PWG

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  • From: Rongrong Ma <marr AT rcf.rhic.bnl.gov>
  • To: STAR PWG Convener List <star-pwgc-l AT lists.bnl.gov>, STAR experiment physics discussions <star-phys-l AT lists.bnl.gov>, Tong Liu <tong.liu AT yale.edu>, STAR centrality focus group <star-centrality-l AT lists.bnl.gov>, aparin via Star-lfsupc-l <star-lfsupc-l AT lists.bnl.gov>, star-cf-l AT lists.bnl.gov, "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: [Star-cf-l] Run19 19.6 GeV centrality definition available in StRefMultCorr
  • Date: Thu, 17 Mar 2022 15:14:12 -0400

Dear All

The latest StRefMultCorr class with Run19 19.6 GeV centrality definition has
now been merged into the main branch, and is available on RCF in DEV
(/afs/rhic.bnl.gov/star/packages/DEV/StRoot/StRefMultCorr).

IMPORTANT: please pay close attention to the example code provided by Grigory
(/star/u/gnigmat/soft/u/refMultCorr/checkStRefMultCorr.C). In particular,
users need to call functions in StRefMultCorr to check bad run and reject
pileup events in their own codes. We will work on automating these checks
within the StRefMultCorr class after QM.

Thanks.

Best
Rongrong

> On Mar 16, 2022, at 3:43 PM, Rongrong Ma via Star-pwgc-l
> <star-pwgc-l AT lists.bnl.gov> wrote:
>
>
>
>> Begin forwarded message:
>>
>> From: Grigory Nigmatkulov via Star-phys-l <star-phys-l AT lists.bnl.gov>
>> Subject: [Star-phys-l] Update of the StRefMultCorr
>> Date: March 16, 2022 at 3:20:57 PM EDT
>> To: STAR centrality focus group <star-centrality-l AT lists.bnl.gov>, STAR
>> experiment physics discussions <star-phys-l AT lists.bnl.gov>, Tong Liu
>> <tong.liu AT yale.edu>
>> Reply-To: Grigory Nigmatkulov <nigmatkulov AT gmail.com>, STAR experiment
>> physics discussions <star-phys-l AT lists.bnl.gov>
>>
>> Dear All,
>>
>> The StRefMultCorr package has been updated. Many thanks to all
>> contributors.
>>
>> We are checking the codes now (currently in the StRefMultCorr_AuAu19p6
>> branch)
>> and those should be merged to the main branch of our git repository
>> (https://github.com/star-bnl/star-sw), where one can find the latest
>> stable codes of STAR, soon.
>>
>> The current code update contains:
>> - Centrality definition for 19.6 GeV
>> - Corrected calculations of isobar trigger efficiency.
>>
>> Steps to obtain the codes:
>> 1. Clone repository (if you did not have codes from git)
>> git clone git AT github.com:star-bnl/star-sw.git
>> You can also find some instructions here:
>> https://drupal.star.bnl.gov/STAR/system/files/smirnov_star_collaboration_meeging_2022.pdf
>>
>> Then go to the directory:
>> cd star-sw/
>>
>> 2. In case your version of code is outdated pull the latest main
>> branch:
>> git pull
>>
>> 3. Switch to the StRefMultCorr_AuAu19p6 branch (this step will not be
>> needed
>> after the codes will be merged to the main branch):
>> git checkout StRefMultCorr_AuAu19p6
>>
>> 4. Copy the StRefMultCorr to your StRoot directory with analysis codes
>> cp -r StRoot/StRefMultCorr /path/to/your/StRoot
>>
>> 5. Compile the codes (for example, with the standard cons) and use.
>>
>>
>> Also for the 19.6 GeV dataset there were some modifications. The working
>> example of the macro can be found here:
>> /star/u/gnigmat/soft/u/refMultCorr/checkStRefMultCorr.C
>>
>> If you have any questions please let me know.
>>
>> Cheers,
>> Grigory
>>
>>
>> _______________________________________________
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>> Star-phys-l AT lists.bnl.gov
>> https://lists.bnl.gov/mailman/listinfo/star-phys-l
>
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  • [Star-cf-l] Run19 19.6 GeV centrality definition available in StRefMultCorr, Rongrong Ma, 03/17/2022

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