Run12 pp500 Relative luminosity and Polarization
Updated on Thu, 2018-06-07 09:46. Originally created by jhkwas on 2018-06-07 09:42.PWG Review Summer 2018: ongoing analyses and upcoming PWGC previews
Updated on Thu, 2019-03-07 15:25. Originally created by yezhenyu on 2018-06-07 07:02.Effects of weak TDC butterworth filter on expected rates.
Updated on Wed, 2018-06-06 19:38. Originally created by bsumma on 2018-06-06 19:38.
HFT embedding request for non-prompt D0
Updated on Sat, 2018-07-14 13:04. Originally created by xlchen on 2018-06-06 10:18.
AUM18 Open Heavy Flavor
Updated on Wed, 2018-06-06 10:05. Originally created by xgn1992 on 2018-06-06 10:05.
AOB
Updated on Wed, 2018-06-06 10:20 by testadmin. Originally created by jeromel on 2018-06-06 10:04.Speaker : All ( All )
Talk time : 12:20, Duration : 00:20
- Update on the picoDST production bookeeping speed (problem You do not have access to view this node )
A case for re-produciton of dAu 200GeV and 62.4GeV for tracking without HFT
Updated on Wed, 2018-06-06 09:02 by slhuang. Originally created by jeromel on 2018-06-06 08:57.Speaker : Shengli Huang ( SUNY-SB )
Talk time : 12:00, Duration : 00:20
Software and Computing Meeting
Updated on Wed, 2018-06-06 08:56 by testadmin. Originally created by jeromel on 2018-06-06 08:56.1-189, SRN, at 16:00 (GMT), duration : 01:00
| Time | Talk | Presenter |
|---|---|---|
| 12:00 | A case for re-produciton of dAu 200GeV and 62.4GeV for tracking without HFT ( 00:20 ) 1 file | Shengli Huang (SUNY-SB) |
| 12:20 | AOB ( 00:20 ) 0 files | All (All) |
STAR Program beyond BES-II
Updated on Wed, 2018-06-06 08:00. Originally created by xzb on 2018-06-06 07:59.Reference
Speaker : Elke Aschenauer
Talk time : 15:30, Duration : 00:30
https://drupal.star.bnl.gov/STAR/system/files/STAR.forward.eca_.pptx
RHIC & AGS Users' Meeting Draft Slides
Updated on Mon, 2018-06-11 17:47. Originally created by jkadkins on 2018-06-05 20:56.Versions are as follows:
v2: Initial upload, and what was sent around to the PWG.
RHIC-AGS-18 poster
Updated on Sat, 2018-06-09 11:54. Originally created by amani on 2018-06-05 18:26.
Prospectus (current)
Updated on Tue, 2018-06-05 16:27. Originally created by djs232 on 2018-06-05 16:27.Update 06.05.2018 -- Run 9 pp: unfolding results (R = 0.3, charged pi0 jets)
Here I present the unfolded recoil jet spectrum using the new response matrix discussed in this post:
Update 06.05.2018 -- Run 9 embedding: (new) response matrix profile check
I realized yesterday that the profile on the response matrix I had shown to JetCorr was using the wrong axis:
Update 06.05.2018 -- Run 9 embedding: closure tests using new matching algorithm
After modifying the paticle-to-detector-level matching algorithm we had been using (see link below), I performed several closure tests.
Update 06.05.2018 -- Run 9 embedding: new matching algorithm
We recently discovered that I wasn't handling the detector-to-particle matching in the best manner. What tipped us off was the (very small) population of jets at large 'pTdetector' but small 'pT
Update 06.05.2018 -- Charge vs. Full Check in Pythia
To illustrate the difference between charged and full jets, I had been using a very old plot I had generated in Pythia. Here's a new one I made for the Annual User's Meeting which looks much nic