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star-hp-l - Re: [Star-hp-l] STAR presentation by Jakub Ceska for Quark Matter 2023 submitted for review

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  • From: Barbara Trzeciak <barbara.trzeciak AT gmail.com>
  • To: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>, STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
  • Cc: webmaster AT star.bnl.gov
  • Subject: Re: [Star-hp-l] STAR presentation by Jakub Ceska for Quark Matter 2023 submitted for review
  • Date: Fri, 21 Apr 2023 23:34:08 +0200

Hi Jakub, Brennan,

I sign off with minor comments:

- Measuring the dependence of self-normalised quarkonium yield dependence on charged particle multiplicity -> Measuring the dependence of self-normalised quarkonium yield on charged particle multiplicity
- with respect to charged particle multiplicity ->  with respect to self-normalised charged particle multiplicity

Cheers,
Barbara

On Fri, Apr 21, 2023 at 1:56 PM Nihar Sahoo via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:
Hello Jakub,

Thank you for your updated abstract.
I don't have further comments.
I sign off.

Cheers
Nihar

On 2023-04-20 19:27, Ceska, Jakub wrote:
> Dear Nihar,
>
>  thank you for your comments. I have uploaded a new version of the
> abstract incorporating Barbara's comments and we feel that most of
> your comments have been addressed. Would you be so kind as to check
> the new version if it is okay?
>
>  Best regards,
> Jakub
>
> -------------------------
>
> Od: Star-hp-l <star-hp-l-bounces AT lists.bnl.gov> za uživatele Nihar
> Sahoo via Star-hp-l <star-hp-l AT lists.bnl.gov>
> Odesláno: čtvrtek 20. dubna 2023 15:02
> Komu: webmaster AT star.bnl.gov <webmaster AT star.bnl.gov>; STAR HardProbes
> PWG <star-hp-l AT lists.bnl.gov>
> Předmět: Re: [Star-hp-l] STAR presentation by Jakub Ceska for Quark
> Matter 2023 submitted for review
>
> Hello Jakub,
>
> Please find my comments on your nice abstract.
>
> General:
> Please use Psi -> $\psi$
> and p+p -> $p$+$p$
>
> Title, Measurement of Upsilon and J/Psi multiplicity dependent
> production in p + p = √s = 510GeV ->
> "Measurement of multiplicity dependent Upsilon and J/Psi production at
>
> √s = 510 GeV in p + p collisions at STAR "
>
> "Proposed explanatory mechanisms, including multi-parton interactions,
>
> string screening, and higher gluon radiation are discussed, as well as
>
> the guidance this measurement and related probes provide to model
> calculations." Not clear. Please rephrase.
>
> Herein we present measurements of -> Herein, we present the
> measurements
> of
>
> in 510 GeV p+p collisions -> at √s = 510 GeV in p+p collisions
> include transverse momentum -> include the transverse momentum
>
> The presented analysis utilises the largest sample of quarkonia the
> STAR
> experiment has obtained from p+p collisions in the dielectron channel,
>
> therefore both increasing precision and extending the reach into
> higher
> multiplicity.
> -> In this measurement, the dielectron channel is used to reconstruct
> quarkonia utilizing high statistics p+p data for the precision
> measurement as well as to achieve the higher multiplicity events in
> the
> STAR experiment.
>
> At the end, you could consider to add "Finally, we compare the data
> with
> the Monte Carlo model predictions and discuss their implications." or
> Something similar.
>
> Cheers
> Nihar
>
> On 2023-04-19 19:39, webmaster--- via Star-hp-l wrote:
>> Dear Star-hp-l AT lists.bnl.gov members,
>>
>> Jakub Ceska (ceskajak AT fjfi.cvut.cz) has submitted a material for a
>> review,
>> please have a look:
>> https://drupal.star.bnl.gov/STAR/node/63484
>>
>> 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
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