STAR Flow, Chirality and Vorticity PWG

["Duckworth, Emilie" <educkwor AT kent.edu>]

 ShinIchi, 

the 7.7 resolution was not updated because the excess proton v1 measurement was already preliminary, only the 9.2, 11.5, 17.3, and 27 gev resolutions were updated. Also, the largest resolution was the 9.2, and that saw the largest change in slope, as can be seen in the attached graph. (clearer datapoints are new, faded ones are old).

Emmy

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From: EsumiShinIchi <esumi.shinichi.gn AT u.tsukuba.ac.jp>
Sent: Wednesday, May 8, 2024 9:02 PM
To: STAR Flow, Chirality and Vorticity PWG <star-fcv-l AT lists.bnl.gov>
Cc: Duckworth, Emilie <educkwor AT kent.edu>
Subject: EXT: Re: [Star-fcv-l] FCV PWG meeting on 08/May/2024 Wed. 9:30 AM EDT

 

Dear Emmy

The resolution seems to be reasonable now, so the final results should be somewhat 

larger now compared to yesterday (since the resolution has been overestimated yesterday), 

however the final results are mostly unchanged. I see some small changes just for some of 

the energies with some small increase, but not much for 7.7GeV, where I was expecting 

the largest change with the highest resolution? Maybe you can make sure the change 

from yesterday for the each points in your page 23...

Best regards, ShinIchi

On May 9, 2024, at 6:29, Duckworth, Emilie via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:

Here is my updated preliminary request with the new resolution correction.

Emmy

---

From: Duckworth, Emilie
Sent: Monday, May 6, 2024 4:54 PM
To: star-fcv-l AT lists.bnl.gov <star-fcv-l AT lists.bnl.gov>
Subject: Re: [Star-fcv-l] FCV PWG meeting on 08/May/2024 Wed. 9:30 AM EDT

 

I would like to submit my CPOD presentation for review and request preliminary status for the plots I plan to show. Please see attached.

Emmy

<preliminary_request_pwg_presentation_2024-05-08.pptx>_______________________________________________
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