STAR HardProbes PWG

[wy157543 AT mail.ustc.edu.cn]

Hi Barbara,

Thank you for the nice comments. This is the new version, please have a look:

https://drupal.star.bnl.gov/STAR/system/files/QM2023_merge_v7.pdf

best,

Yan

-----原始邮件-----
发件人:"Barbara Trzeciak" <barbara.trzeciak AT gmail.com>
发送时间:2023-04-24 17:46:10 (星期一)
收件人: wy157543 AT mail.ustc.edu.cn, "STAR HardProbes PWG" <star-hp-l AT lists.bnl.gov>
抄送: "Yi Yang" <yiyang0429 AT gmail.com>, webmaster AT star.bnl.gov
主题: Re: [Star-hp-l] STAR presentation by Yan Wang for Quark Matter 2023 submitted for review

Hi Yan,

I have last minor comments:

- L2: Quarkonia productions is an interplay of -> Production of quarkonia involves

- L8: observations -> observables

Cheers,

Barbara

On Mon, Apr 24, 2023 at 9:36 AM wy157543--- via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

Hi Yi,

Thank you for the nice comments. This is the new version, please have a look:

https://drupal.star.bnl.gov/STAR/system/files/QM2023_merge_v6.pdf

Best,

Yan

-----原始邮件-----
发件人:"Yi Yang" <yiyang0429 AT gmail.com>
发送时间:2023-04-24 07:56:31 (星期一)
收件人: wy157543 AT mail.ustc.edu.cn
抄送: "STAR HardProbes PWG" <star-hp-l AT lists.bnl.gov>, webmaster AT star.bnl.gov
主题: Re: Re: [Star-hp-l] STAR presentation by Yan Wang for Quark Matter 2023 submitted for review

Hi Yan,

Thank you very much for addressing my comments and the updated version looks good to me. 

Only one minor minor thing: 

 L6: and polarization --> , and polarization

Cheers,

Yi

On Sun, Apr 23, 2023 at 7:25 PM <wy157543 AT mail.ustc.edu.cn> wrote:

Hi Yi and Barbara,

Thank you for the nice comments. This is the new version, please have a look:

https://drupal.star.bnl.gov/STAR/system/files/QM2023_merge_v5.pdf

best,

Yan

-----原始邮件-----
发件人:"Yi Yang via Star-hp-l" <star-hp-l AT lists.bnl.gov>
发送时间:2023-04-23 08:45:23 (星期日)
收件人: webmaster AT star.bnl.gov, "STAR HardProbes PWG" <star-hp-l AT lists.bnl.gov>
抄送:
主题: Re: [Star-hp-l] STAR presentation by Yan Wang for Quark Matter 2023 submitted for review

Hi Yan, Dandan, and Te-Chuan,

Thanks a lot for providing the merged abstract. I have some minor comments for your consideration. 

 - General 1: I am fine with the current abstract, but it reads not that exciting. I would think that it would be good to provide a bigger picture in the beginning, for example, to understand the quarkonium production mechanism and properties of QGP, we need to consider all aspects, such as the yield suppressions, sequential melting, polarization, so on. Precision measurements are also important, so high statistics isobar data provide us this opportunity. Just something for your consideration. 

 - General 2: I think this abstract is too focused on Psi(2S) (especially in the second paragraph). I agree that this is one of the most important results), but it would be good to add a bit more descriptions on Upsilon and J/psi polarization.  

 - I believe both Upsilon and J/psi polarization are also using e+e- channel, so it is a bit weird if you only mentioned it for Psi(2S)

 - L15: heavy ion --> heavy-ion 

 

Cheers,

Yi

On Mon, Apr 17, 2023 at 11:02 PM webmaster--- via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

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

Yan Wang (wy157543 AT mail.ustc.edu.cn) has submitted a material for a review, 
please have a look:
https://drupal.star.bnl.gov/STAR/node/63401

Deadline: 2023-05-01
---
If you have any problems with the review process, please contact 
webmaster AT www.star.bnl.gov
_______________________________________________
Star-hp-l mailing list
Star-hp-l AT lists.bnl.gov
https://lists.bnl.gov/mailman/listinfo/star-hp-l

_______________________________________________
Star-hp-l mailing list
Star-hp-l AT lists.bnl.gov
https://lists.bnl.gov/mailman/listinfo/star-hp-l