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star-hp-l - Re: [Star-hp-l] STAR presentation by Isaac Mooney for Hard Probes 2023 submitted for review

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Subject: STAR HardProbes PWG

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  • From: Barbara Trzeciak <barbara.trzeciak AT gmail.com>
  • To: "Ma, Rongrong" <marr AT bnl.gov>, STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
  • Cc: Yi Yang <yiyang0429 AT gmail.com>, Te-Chuan Huang <tchuang.phys AT gmail.com>
  • Subject: Re: [Star-hp-l] STAR presentation by Isaac Mooney for Hard Probes 2023 submitted for review
  • Date: Fri, 24 Mar 2023 10:20:16 +0100

Hi Isaac,

I have one last comment on your nice poster and sign off.

Increase font size (axis' title, text inside) of the q2 plots.

Cheers,
Barbara


On Fri, Mar 24, 2023 at 1:31 AM Ma, Rongrong via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:
Hello Te-Chuan

This is great. Thanks. 

Best
Rongrong

On Mar 23, 2023, at 7:51 PM, Te-Chuan Huang <tchuang.phys AT gmail.com> wrote:

Hi Rongrong,

I think the link below is the original source of these STAR pictures.

Cheers,
Te-Chuan


On Mar 23, 2023, at 6:36 PM, Mooney, Isaac via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:

Hi Rongrong,

Thanks for the quick comments. I’ve implemented them (as well as Helen’s comment) in v2 on the node now. I’m also attaching the STAR detector figure, but the resolution I have it in is not the best. Maybe others have a better version.

Thanks,
Isaac

<STARdetector.png>


On Mar 23, 2023, at 6:36 PM, Ma, Rongrong <marr AT bnl.gov> wrote:

Hello Isaac

In the interest of time, here are some comments for you consideration. 

General
- Since you list BNL as one of your affiliations, I suggest to add the BNL logo as well.

ABSTRACT
- transfer -> transfers
- to small systems and Au+Au results -> to both small and large collision systems

MOTIVATION
- Energy Density of overlap -> Energy density of overlapping

THE STAR EXPERIMENT
- Could you send me this STAR detector figure in high-resolution? I can collect it on our central page. Thanks. 

CHARGED HADRON SUPPRESSION IN ISOBAR COLLISIONS
- high p_T tracks -> higher p_T tracks
- Is it mis-binning of centrality or N_coll does not scale with N_hard in peripheral events?

CONCLUSIONS
- Hadron yields show -> Hadron suppression shows
- on the system geometry -> on the collision geometry

Best
Rongrong

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:
https://nam12.safelinks.protection.outlook.com/?url="https%3A%2F%2Furldefense.com%2Fv3%2F__https%3A%2F%2Fnam12.safelinks.protection.outlook.com%2F%3Furl%3Dhttps*3A*2F*2Fdrupal.star.bnl.gov*2FSTAR*2Fnode*2F63045%26data%3D05*7C01*7Cisaac.mooney*40yale.edu*7Cdda688a1c57646af5be708db2ae1df22*7Cdd8cbebb21394df8b4114e3e87abeb5c*7C0*7C0*7C638150921821730650*7CUnknown*7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0*3D*7C3000*7C*7C*7C%26sdata%3DFm63S*2B8QeFS6O6lwDFa8S5FpGqHrH7Nb07ZwM5e3o04*3D%26reserved%3D0__%3BJSUlJSUlJSUlJSUlJSUlJSUlJSUlJSU!!P4SdNyxKAPE!HBkMH4TmY15oO3aEPy7c5bhaWBZDtv-Cg6HhnTFgaAdZsEJ6PZ7UcrIE5AFPA-HJ6cY8WwDcsUafJN3olm7ywc8bqVJon_A%24&data=05%7C01%7Cisaac.mooney%40yale.edu%7C6168dc0848344d09708e08db2bef1516%7Cdd8cbebb21394df8b4114e3e87abeb5c%7C0%7C0%7C638152078074583610%7CUnknown%7CTWFpbGZsb3d8eyJWIjoiMC4wLjAwMDAiLCJQIjoiV2luMzIiLCJBTiI6Ik1haWwiLCJXVCI6Mn0%3D%7C3000%7C%7C%7C&sdata=LHxwymdjAKw8r4tV3tNwug8I%2FP4S0vcczSRkWzmIfN0%3D&reserved=0 

Deadline: 2023-03-26
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