STAR HardProbes PWG

[tc88qy <tc88qy AT rcf.rhic.bnl.gov>]

Hi Yu-ming
  can you send out eps or pdf file rather than svg file?
It would be very helpful that you can make one or two sentence for page 
13.

Thanks
Qian Yang


On 2022-06-09 14:59, Yu-Ming Liu wrote:
> Hi Qian and Barbara,
>
> sorry for the late reply.
> Attached are the svg files of plots which Qian used in p13, v2 as a
> function of pT in 20-60% centrality and v2 in pT 4-10 GeV/c in
> 0-80%centrality.
>
> Best,
> Yu-Ming
>
> tc88qy via Star-hp-l <star-hp-l AT lists.bnl.gov> 於 2022年6月8日
> 週三 下午7:06寫道：
>
> > Hi Barbara and all
> >
> > After a local STAR group rehearsal, I updated the new version in
> > the
> > same link (v4)
> > Please send out your comments. Thanks
> >
> > Qian Yang
> >
> > On 2022-06-05 09:50, tc88qy via Star-hp-l wrote:
> > > Hi Barbara
> > >
> > > Thanks for your suggestion, Please find my rely inline. and new
> > > version of slides are in the same link
> > >
> > >
> > > Qian Yang
> > >
> > > On 2022-06-04 16:37, Barbara Trzeciak wrote:
> > > > Hi Qian,
> > > >
> > > > thanks for the update. The slides are very nice, please find my
> > > > comments below.
> > > >
> > > > Cheers,
> > > > Barbara
> > > >
> > > > s3 - I would also mention CNM effects
> > > Here I want to more focus on the hot medium effect. so I did not
> > > mention CNM.
> > >
> > > > s4 -  How it affect ->  How is it affected
> > > done
> > > > s5 - w be established -> evolves (?)
> > > done
> > > > s6 - v2 -> v_2
> > > done
> > > > s8 - make the left plot larger
> > > done
> > > > s9- dependence were shown -> dependence is observed
> > > done
> > > > s11 - you can emphasise here precision of the isobar measurement
> > > done
> > > > s13 - it would be good to have better quality plots here. Maybe
> > > > Yu-Ming can prepare example procedure figures with better
> > graphics.
> > > > Also, are these efficiency weighed, is there some physics one can
> > > > extract ?
> > > Sure, It will be good that Yu-Ming can prepare one page of slides
> > for
> > > the procedure.
> > > The graphic is from Yu-Ming's preliminary request slides, I think
> > it
> > > is efficiency weighted.
> > >
> > > > s14 - I think it makes more sense to compare 0-80% isobar to
> > 0-80%
> > > > Au+Au - so to have the Au+Au results on the left plot. But let's
> > also
> > > > see what others think and we can then decide on the final version
> > of
> > > > these plots.
> > > > Also, for the 20-60% range please keep in mind that Yu-Ming might
> > have
> > > > his HT results early next week - in this case please update the
> > plot.
> > > > s15 - since we have higher pT results it would be nice to have
> > here
> > > > also the integrated v2 for higher pT > 4 GeV/c from the HT.
> > >
> > > ok
> > >
> > > > s15 - it's not so obvious to me how much better precision we have
> > in
> > > > isobar compared to Au+Au. Is it possible to combine Au+Au for pT
> > < 4
> > > > GeV/c ? Also, I think it would be better not to combine stat. and
> > sys.
> > > > uncertainties for Au+Au results (also for the other comparison),
> > it
> > > > might show better statistical differences between the two
> > results.
> > > The combination is not just combine the final physics data point,
> > But
> > > do the extraction from the beginning.
> > > and the stat. and sys. are all needs re-calculation.
> > > I did not put sys. uncertainties for the Au+Au results, the error
> > bars
> > > are just stat. uncertainties.
> > > But the sys. uncertainties is small for Au+Au.
> > >
> > > > s15 - for low pT, i.e. ~< 1 GeV/c, we expect 0 v2 because of the
> > mass
> > > > effect. If it's fast, can you calculate integrated v2 for pT > 1
> > GeV/c
> > > > ?
> > > I need to do some change to have this results. Let's us see, If I
> > can
> > > have the final results next week.
> > > > On Fri, Jun 3, 2022 at 8:54 AM tc88qy via Star-hf-l
> > > > <star-hf-l AT lists.bnl.gov> wrote:
> > > >
> > > > > Hello All
> > > > >
> > > > > As we discussed in yesterday's HP meeting. I have updated the
> > > > > slides to
> > > > > a new version.
> > > > > Please find in the same link. Your comments and suggestion are
> > > > > welcome.
> > > > >
> > > > > Qian Yang
> > > > >
> > > > > On 2022-05-31 19:27, webmaster--- via Star-hf-l wrote:
> > > > > > Dear star-hf-l AT lists.bnl.gov members,
> > > > > >
> > > > > > Qian Yang (qianyangstar AT gmail.com) has submitted a material for
> > a
> > > > > > review,
> > > > > > please have a look:
> > > > > > https://drupal.star.bnl.gov/STAR/node/59787
> > > > > >
> > > > > > ---
> > > > > > If you have any problems with the review process, please
> > contact
> > > > > > webmaster AT www.star.bnl.gov
> > > > > > _______________________________________________
> > > > > > Star-hf-l mailing list
> > > > > > Star-hf-l AT lists.bnl.gov
> > > > > > https://lists.bnl.gov/mailman/listinfo/star-hf-l
> > > > > _______________________________________________
> > > > > Star-hf-l mailing list
> > > > > Star-hf-l AT lists.bnl.gov
> > > > > https://lists.bnl.gov/mailman/listinfo/star-hf-l
> > > _______________________________________________
> > > Star-hp-l mailing list
> > > Star-hp-l AT lists.bnl.gov
> > > https://lists.bnl.gov/mailman/listinfo/star-hp-l
> > _______________________________________________
> > Star-hp-l mailing list
> > Star-hp-l AT lists.bnl.gov
> > https://lists.bnl.gov/mailman/listinfo/star-hp-l

Attachment: cosdis_pt4to5_sthf_SQM.svg
Description: image/svg

Attachment: cosdis_pt3to4_sthf_SQM.svg
Description: image/svg

Attachment: v2_yuming2.root
Description: Binary data