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star-hp-l - Re: [Star-hp-l] STAR presentation by Andrew Tamis for ECCF submitted for review

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Subject: STAR HardProbes PWG

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  • From: Yi Yang <yiyang0429 AT gmail.com>
  • To: Andrew Tamis <andrew.tamis AT yale.edu>
  • Cc: STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>, Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>, webmaster AT star.bnl.gov
  • Subject: Re: [Star-hp-l] STAR presentation by Andrew Tamis for ECCF submitted for review
  • Date: Mon, 8 Jul 2024 05:39:42 +0800

Hi Andrew,

Thanks a lot! Just for the record, I don't have any further comments on it.

Cheers,
Yi

On Mon, Jul 1, 2024 at 11:56 PM Andrew Tamis <andrew.tamis AT yale.edu> wrote:
Hello Yi and Nihar,

Thank you very much for the comments, I have implemented them and uploaded a new version.

For Yi's point about defining the turnover point, i think this is definitely possible but most likely not before the workshop, and I will work on it for the paper.  For Nihar's slide 5 comment, i meant to imply that the initiating parton changes where this parton/hadron transition occurs, I have updated text from "transition shift" to transition region shifts based on initiator

Best,
Andrew

On Mon, Jul 1, 2024 at 5:16 AM Nihar Sahoo via Star-hp-l <star-hp-l AT lists.bnl.gov> wrote:
Hello Andrew,

Your presentation slides look good to me. I have some comments below.
With these implemented I sign off.

SLide5: Quark, gluon fragmentation differences transition shift -> Could
you please elaborate? is this different from hadron-pardon transition?

SLide12: left top (small) text equation -> it would be good to make it
clear and large; and also please write down full _expression_.


Best
Nihar


On 2024-06-30 02:06, Yi Yang via Star-hp-l wrote:
> Hi Andrew,
>
> Thanks a lot for the nice slides. I have some minor comments for your
> consideration.
>  - p4: I still think there should be a way to determine the turnover
> point, you probably can use the similar method from AMS to do it
> (Figure 4,
> https://ams02.space/physics/towards-understanding-origin-cosmic-ray-positrons
> [1])
>  - p5: STAR Result --> STAR result
>  - p5: this plot is a bit busy, and it's not easy to see the STAR
> points. Is it possible to make the STAR points in red?
>  - p7: By just reading the slides, it seems a bit strange to have this
> rc here, but probably you can make a nice transition. Please add the
> definition of rc in this slide.
>
> Cheers,
> Yi
>
> On Sat, Jun 29, 2024 at 11:56 PM webmaster--- via Star-hp-l
> <star-hp-l AT lists.bnl.gov> wrote:
>
>> Dear Star-hp-l AT lists.bnl.gov members,
>>
>> Andrew Tamis (andrew.tamis AT yale.edu) has submitted a material for a
>> review,
>> please have a look:
>> https://drupal.star.bnl.gov/STAR/node/68233
>>
>> Deadline: 2024-07-08
>> ---
>> 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
>> https://lists.bnl.gov/mailman/listinfo/star-hp-l
>
>
> Links:
> ------
> [1]
> https://urldefense.com/v3/__https://ams02.space/physics/towards-understanding-origin-cosmic-ray-positrons__;!!P4SdNyxKAPE!CycTC4dAYpOukuBdZlWGapx5Rxt5C4IUOW1ehemuMBP_8HodDmHWnQqV-6ZHL2E-8ONIRV5zDBFWqDlnY9QkK9J9AQ$
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