STAR HardProbes PWG

[Sooraj Radhakrishnan <skradhakrishnan AT lbl.gov>]

Hi Andrew,

   Thanks for preparing these nice slides. Since you show detector level and generator level PYTHIA distribution are quite similar, I wonder if the results should be labelled STAR Preliminary, as they can be argued to be close to the physics results. Do you want to show the data also at DNP or just the PYTHIA results and give some performance plots for data?

thanks

Sooraj

On Mon, Oct 17, 2022 at 6:27 AM 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/61351

Deadline: 2022-10-27
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Sooraj Radhakrishnan

Research Scientist,

Department of Physics

Kent State University

Kent, OH 44243

Physicist Postdoctoral Affiliate

Nuclear Science Division
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road

Berkeley, CA 94720

Ph: 510-495-2473

Email: skradhakrishnan AT lbl.gov