STAR HardProbes PWG

[Yi Yang <yiyang0429 AT gmail.com>]

Hi Veronica,

Thanks a lot for the updated version. I don't have any further comments (I think after addressing Nihar and Issac's comments are good enough!). 

Regarding the conclusion, I think Issac's suggestion is a good one " "R_{pAu} for J/\psi is in agreement with RdAu as measured in PHENIX, and consistent with models which only include CNM effects.". You can consider using it!

Cheers,

Yi

On Sat, May 13, 2023 at 11:09 AM Veronica Verkest <vverkest AT gmail.com> wrote:

Hello Yi,

Thanks for another thorough revision--especially concerning conclusions about J/psi measurements and CNM effects, which are not as intuitive to me as jets. I also appreciate the attention to style/structure. I updated the PDF on Drupal and in addition to your revisions, I slightly modified the sentences on lines 38 and 87. The 4-page limit is not an issue, I just like to make our plots bigger when possible. In addition, the title page photo is optional, but it does not add as many lines as its height, per LaTeX styling.

Thanks,

Veronica

On Fri, May 12, 2023 at 10:18 PM Yi Yang <yiyang0429 AT gmail.com> wrote:

Dear Veronica,

Thanks a lot for the updated version. I only have some follow up suggestions for your consideration. 

 - L37: I wanted to say removing "cold nuclear matter", but I typed CNM. Please use CNM here. Sorry about that. 

 - L71: I would use "showing clear CNM effect at low-pT".

 - L105: I understand there is a page limitation, but I would suggest putting the "clear CNM effect at low-pT for J/psi" in the conclusion. 

Cheers,

Yi

On Sat, May 13, 2023 at 4:56 AM Veronica Verkest <vverkest AT gmail.com> wrote:

Hi all,

Yi –– I appreciate all the helpful feedback! I have implemented all of your changes and I have also changed the acknowledgements section to be more specific.

I have uploaded this slightly revised version so that Nihar and Isaac can look it over at their convenience. There is a 4 page limit, so we cannot add quite too much more content anyway.

Thanks,

Veronica

On Fri, May 12, 2023 at 3:38 PM Yi Yang <yiyang0429 AT gmail.com> wrote:

Dear Veronica,

Thank you so much for the nice proceedings. I have some minor comments for your consideration. 

 - L24: Fig. 1 --> Figure 1 

 - L36: remove (CNM) 

 - L43: image --> plot 

 - L44: high-E_T --> high-transverse-energy (high-E_T)

 - L52: image --> plot

 - L54: p_T --> transverse momentum (pT)

 - Figure 3 actually indicates that CNM is observed at low pT < 3 GeV region and it should be mentioned in the text.  

 - L73: the description of the nuclear modification factor should move up to around L62, before talking about the RpA for J/psi. 

 - L75: image --> plot

 - L75: jets --> J/psi

 - L77: need to define Npart 

 - Figure 4: The left plot is RAA for J/psi, should be mentioned in the caption. 

 - L79: since you specifically describe Upsilon here, should you describe J/psi as well somewhere before it? 

 - L81: image --> plot

 - L90: Fig. 5 --> Figure 5

 - L104: should mention J/psi here 

Cheers,

Yi

 

On Sat, May 13, 2023 at 12:26 AM Veronica Verkest via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

Hi all,

In the hustle of recent submissions, I just wanted to send a reminder about my Moriond proceedings (here: https://drupal.star.bnl.gov/STAR/node/63649). The due date is the 15th, which is Monday. I welcome and appreciate any feedback!

Thanks,

Veronica

On Mon, May 8, 2023 at 7:36 PM webmaster--- via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

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

Veronica Verkest (vverkest AT gmail.com) has submitted a material for a review, 
please have a look:
https://drupal.star.bnl.gov/STAR/node/63649

Deadline: 2023-03-25
---
If you have any problems with the review process, please contact 
webmaster AT www.star.bnl.gov
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