STAR Correlations and Fluctuations PWG

[EsumiShinIchi <esumi.shinichi.gn AT u.tsukuba.ac.jp>]

Dear Daniel

Thank you very much for the very nice presentation. I here send you some minor 

comments, that I find your instruction in your earlier pages are quite nice, especially 

how this alpha parameter acts as non-gaussian source shape etc in p5. While I also 

think it would be very good, if you could tell what would be the merit of this 1D Levy 

fitting compared to the usual 3D gaussian source analysis, if you can at least say 

this non-gaussian shape is not just coming from the 3D to 1D conversion/averaging, 

that would have different source sizes depending on the 3 directions. Therefore you 

might like to go to the 3D-Levy as your next step, though… Thanks again. 

Best regards, ShinIchi

2023/10/31 16:04、Kincses Dániel via Star-cf-l <star-cf-l AT lists.bnl.gov>のメール:

Dear Conveners,

My talk is currently scheduled for the first day of the conference (November 6). I would appreciate any comments or suggestions!

Thanks,
Daniel

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Feladó: Star-cf-l <star-cf-l-bounces AT lists.bnl.gov>, meghatalmazó: webmaster--- via Star-cf-l <star-cf-l AT lists.bnl.gov>
Elküldve: 2023. október 26., csütörtök 10:47
Címzett: star-cf-l AT lists.bnl.gov <star-cf-l AT lists.bnl.gov>
Másolatot kap: webmaster AT star.bnl.gov <webmaster AT star.bnl.gov>
Tárgy: [Star-cf-l] STAR presentation by Daniel Kincses for WPCF 2023 submitted for review

 

Dear star-cf-l AT lists.bnl.gov members,

Daniel Kincses (kincses AT ttk.elte.hu) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/65727

Deadline: 2023-11-06
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If you have any problems with the review process, please contact  
webmaster AT www.star.bnl.gov
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