STAR HardProbes PWG

[gaohan_yang <gaohan_yang AT m.scnu.edu.cn>]

Hi, Barbara

Thank you for your valuable comments and patient response.  I have implemented them and uploaded version2 on the Drupal page which can be found in this link:

https://drupal.star.bnl.gov/STAR/system/files/Athic_Upsilon_Production_V2_0.pdf

Please see my detailed responses inline:

|-General suggestion for your consideration: you don't necessarily need to divide your presentation into Au+Au and isobar -> you can show the published results in Au+Au, then isobar and isobar compared to Au+Au, and then model and LHC comparisons at the end.

— I have adjusted the order and content of the slides according to your comments. If you have any other suggestions, please let me know.

|-Why in the table do you specifically show 30-60% for Au+Au and 0-80% for Ru+Ru and Zr+Zr ?

I would rather show for which centrality bins that you have the <N_coll> are similar between the systems.

— Yes, we compared the two systems based on the number of  similar N_parts. Maybe my table didn't explain it clearly. But that's okay, I've removed this slide now.

|-And is it possible to estimate the Upsilon(3S) upper limit for isobars ? 

— Considering the large uncertainties of Y(2S) and negative Y(2S) yield in isobar collisions, estimate the Upsilon(3S) upper limit won't make significant physics impact. We prefer not to draw the Y(3S) upper limit .

Best,

Gaohan

On Thu, Apr 13, 2023 at 11:52 AM webmaster--- via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

Dear Star-hp-l AT lists.bnl.gov members,

Gaohan Yang (gaohan_yang AT m.scnu.edu.cn) has submitted a material for a 
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/63345

Deadline: 2023-04-24
---
If you have any problems with the review process, please contact 
webmaster AT www.star.bnl.gov
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