STAR Protected
Non-photonic electrons in d+Au 2008
I decided to take a first look at non-photonic electrons in d+Au 2008, in an attempt to do e-D0 correlations.
Cuts are mostly the default of the previous e-D0 analyses:
Bulk Correlations Physics Working Group EVO meeting
EVO, STAR Community, at 15:00 (GMT), duration : 01:30
Please upload agenda items, or links to agenda items
2008.10.27 SMD-based shower shape scaling: 25 strips cluster energy, raw vs. data-driven MC
Ilya Selyuzhenkov October 27, 2008
Data sets:
Comparison of spectra run 3 vs run 8
Below is an attempt to look at spectra in run 8 vs run 3 d+Au.
Medium density from IAA
In order to see how well our IAA measurement constrains the medium density in models, I started making a comparison following the method by Jamie Nagle.
STAR Management Meeting
BNL, 50-I-189, at 14:00 (GMT), duration : 01:00
Conference Phone Number: 510 486 7333
Time: 10 - 11 am EDT
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Agenda:
0) Joule targets for FY09 - Bill
1) QM09 speaker discussions - Nu
2) STAR computing plan - Jerome
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Brief Summary:
0) Performance Goal for FY09: # of events to be recorded, 4 weeks at 500 GeV p+p collisions, 11 weeks at 200 GeV p+p collisions.
- 150Hz, 50hr/week, HT/jet patch trigger for W I.D.+M.B., ~120M events for 500 GeV p+p collisions.
- 400+Hz, 63hr/week, ~ 900M events for 200 GeV p+p collisions.
Bernd will discuss this in Spin group for discussions.
2008.10.21 Shower shapes, 5/25 strips cluster energy, raw vs. data-driven MC
Ilya Selyuzhenkov October 21, 2008
Data sets:
STAR incl jets talk - wwj at DNP08
1st draft of inclusive jet talk for DNP08. Figs and text _all_ taken from recent (longer) STAR talks by others (thanks!) and compressed for 10 minute DNP format.
Comparisons between STAR and PHENIX
This is a page that Thomas will edit to work on comparisons between STAR and PHENIX Non-Photonic electrons
2008.10.15 Comparison of gamma-jets from Michael's filtered events vs. old MC samples
Ilya Selyuzhenkov October 15, 2008
Data sets:
Kaon-kaon fitting with momentum resolution
Fitting kaon-kaon correlation functions with momentum resolution
In this page I will show the results of the fit of the experimental kaon-kaon correlation functions (binned directly in sphe