STAR HardProbes PWG

[Helen Caines <helen.caines AT yale.edu>]

Hi Isaac,

 You might have left the meeting at that point, but can you replace the NPart RAA plot with the one Tong has that does not include the PHENX data? Please also send this version to Nihar and Joern for their talk. Its well known that the PHENIX and STAR RAA don’t agree well, so including them in the plot I think muddles the picture about Npart being the driver for the suppression.  

Helen

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On Mar 23, 2023, at 6:10 PM, Mooney, Isaac via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

Hi everyone,

I have addressed all of the helpful comments, in addition to some from the group at Yale, in v1 now on the node. Please let me know if there are any further comments.

Best,

Isaac

On Mar 23, 2023, at 8:04 AM, Barbara Trzeciak <barbara.trzeciak AT gmail.com> wrote:

Hi Isaac,

Nice poster, please see below my minor comments:

Abstract:

ratio of hadron or jet spectra in A+A and p+p collisions called the -> ratio of hadron or jet spectra in A+A and p+p collisions scaled by the number of binary nucleon-nucleon collisions called the

In this talk -> In this poster

ESE

[Done by ALICE; see talk by C. Beattie on 30th] - you can make this smaller and the full reference seems to be missing

→ path length dependence of jet energy loss! - you can use bold or some colour

Cheers,

Barbara

On Thu, Mar 23, 2023 at 11:35 AM Yi Yang via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

Hi Isaac,

No worries and thanks a lot for the nice poster. 

I have some minor comments for your consideration. 

 - The STAR Experiment: is it possible to rearrange the text and picture, like to all text at the top (6 lines) and put the STAR in the bottom, and hope this will make the picture bigger. (Up to you)

 - Charged hadron suppression: could you please add a bullet on each item? Up to you, too. 

 - Event shape engineering: I agree with what Rongrong suggested. 

Cheers,

Yi

On Wed, Mar 22, 2023 at 9:39 AM Mooney, Isaac via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

Hi all,

I’ve posted a draft of the poster. I sincerely apologize for the delay in getting this to the list. I will make every effort to make sure it doesn’t happen again.
Note on the final two plots: the 2D histogram is on the full (Ru) dataset; the v2 plot is the result of a suggestion from the FCV PWG to demonstrate that q2 has some sensitivity to anisotropy, and I will increase the statistics used, probably with the next draft I send out. As this is v2-obs and not the v2 corrected for event plane resolution, it is not a “physics" plot.
For both plots I know there are labels that need to be added, and beautification to be done, but I will also take care of that in the next iteration.

Thanks for your consideration,
Isaac

> On Mar 22, 2023, at 10:29 AM, webmaster--- via Star-hp-l <Star-hp-l AT lists.bnl.gov> wrote:
>
> Dear Star-hp-l AT lists.bnl.gov members,
>
> Isaac Mooney (isaac.mooney AT yale.edu) has submitted a material for a review, 
> please have a look:
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