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star-hp-l - Re: [Star-hp-l] STAR presentation by Brennan Schaefer for HP2024 submitted for review

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Subject: STAR HardProbes PWG

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  • From: Brennan Schaefer <brs521 AT lehigh.edu>
  • To: STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
  • Cc: Barbara Trzeciak <barbara.trzeciak AT gmail.com>, Yi Yang <yiyang0429 AT gmail.com>
  • Subject: Re: [Star-hp-l] STAR presentation by Brennan Schaefer for HP2024 submitted for review
  • Date: Fri, 24 May 2024 09:18:37 -0400

Greetings Barbara, conveners, and HP analyzers, 

   below is a link to the third revision of my abstract for HP2024.

https://drupal.star.bnl.gov/STAR/node/67732

best,


b


On Fri, May 24, 2024 at 3:13 AM Barbara Trzeciak via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:
Hi Brennan,

Could you please address the remaining comments so that the abstract can be pushed to the star-talks and approved.
The submission deadline to the conference is tomorrow.

Thanks,
Barbara

On Thu, May 23, 2024 at 11:24 AM Barbara Trzeciak <barbara.trzeciak AT gmail.com> wrote:
Hi Brennan,

In addition to the comments from conveners, I have the following suggestions.

I would not say "consistent with" - this is under study what concerns this abstract. I would just write that the faster than linear rise was observed at 200 GeV, 7 and 13 TeV, and that with your new results you can test it and improve.
Which brings me to the second comment. It's not clear from the last sentence that the measurement to be shown in this talk extends the measured previous range. Also, "extending the measurement normalized multiplicity range"

Cheers,
Barbara

On Thu, May 23, 2024 at 9:46 AM Yi Yang via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:
Hi Brennan,

I have one comment on your updated version (sent in the other thread).

You mentioned that "The investigation of quarkonium production allows for the study of the properties of strongly interacting matter, such as interactions with the quark-gluon plasma and nucleonic gluon content." However, your analysis is for p+p collisions, so it would be good to have a connection between p+p and QGP.

Cheers,
Yi

On Wed, May 22, 2024 at 11:57 AM Brennan Schaefer via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:
Hi Barbara,

Yes, I’ve uploaded a second version of the abstract.  Following the comments, instead of a revision, a near complete rewrite was necessary.


all the best,


b


On Wed, May 22, 2024 at 5:40 AM Barbara Trzeciak via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:
H Brennan,

Any updates on your abstract ?

Cheers,
Barbara

On Tue, May 14, 2024 at 2:19 PM Nihar Sahoo via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:
Hello Brennan,

Thank you for your nice abstract.
A few comments can be found below.

1) it would be good to mention what kinematic range this measurement
will be reported. For instance, pT, eta, etc.
2) thereby increasing precision and extending the reach into higher
multiplicity. -> It would be better to mention, if possible, why it is
important to explore high multiplicity range?


Best
Nihar

On 2024-05-11 02:09, webmaster--- via Star-hp-l wrote:
> Dear Star-hp-l AT lists.bnl.gov members,
>
> Brennan Schaefer (brennanschaefer AT hotmail.com) has submitted a material
> for a
> review, please have a look:
> https://drupal.star.bnl.gov/STAR/node/67732
>
> Deadline: 2024-05-25
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov
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