STAR HardProbes PWG

[Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>]

Hello Diptanil,

Nice slides.
Please find some comments below.

Slide5:

Jet energy is redistributed to large distances from the jet axis in 
medium -> Jet energy is redistributed to large angles from the jet axis 
in medium (as we use kinematic phase space in jet recon)

Slide6:
…different aspects o jet fragmentation -> Not clear what are those 
“aspects”, for example?

Slide7,8: These slides come abruptly, can you try to make a story to 
combining both jet angularity and D^0+jet in one slide

Slide9: That upward arrow at 1, Can you make downward arrow? Because it 
seems you are interested in POWHEG than data.
Slide10: 		is smaller at STAR for a given … -> 		is smaller in AuAu 
sNN=200 GeV collisions for a given
[STAR is not a collision system]

SLide22: Why have not you updated uniform systematic uncertainty for 
right most panel? You need to update with your revised plot here.

Slide24: This slide is not clear. Please mention what point you want to 
make here.

Slide25:
_ No radial profile modification for D0 in jets -> No radial profile 
modification for D0 in jets in central Au+Au collisions

Your Summary last slide should be Slide24 with similar comment. Then 
don’t discuss at the end. Otherwise the flow is not ending at the end.

Best
Nihar








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