STAR Protected
Rho reconstruction simulation study with FMS+FHC
I studied the rho+ reconstruction with 10M pythia+GSTAR simulation events.
Unable to find agreement with prior values (again)
The cross section for the BHT3 trigger is likely to change over time, both from beam-related backgrounds we can't identify and from changes in the gains of the individual towers which we can'
Calibrations status (2010-01-13)
Updating status and progress of the Run 9 calibrations since my last report:
7: 2010/JAN/12 J/Psi dAu2010 embedding on disk
The old J/Psi embedding files are on disk for period january 2010:
/eliza14/star/starprod/embedding/production_dAu/Jpsi_10{3-7}_1229459741
It is about 150 GB of files
Status - STAR Upgrades
Updated on Sun, 2010-01-17 10:13 by videbaks. Originally created by sichterm on 2010-01-11 18:37.Speaker : Nu Xu for Flemming Videbaek
Talk time : 10:00, Duration : 00:20
Trying to finalize the BHT3 xs
I've written about the somewhat double-gaussian approach to fitting the BHT3 vernier scans already, so this is just a brief addendum:
Austin mtg jet talk January 2010
Draft of pp jet talk for Friday 1/15/10. pdf does not preserve animations.
Near final version v2.
FMS Calibration Tools
Hi,
Event by event comparison between Energy distributions and fitted distributions (2 photon events). These are events that
Comparison of high pT Gamma Candidates in filtered MC vs. 2006 data
Information
MC is generated using a gamma filter, modified from one by Mike B. I use the following cuts:
2010.01.08 EEMC response 2006 vs. 2009: phi cuts
EEMC migration plots with cuts on TPC sector boundaries
Table of BHT3 luminosities
I've attached a table of the BHT3 luminosities in the L2W dataset.
2010.01.07 EEMC response to single photons with y2006h vs y2009a geometries
Monte-Carlo setup
- Throwing one photon per event
- Full STAR y2006h/y2009a configurations
- Throw particles flat in eta (1.08, 2.0), phi (0, 2pi), and en
HOWTO: Get the list of particle IDs from ...
starsim> gprint part
starsim> call pylist(11)