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:

Panic Talk on Eta An

This differs from Len's only in the first 4 slides.

Bulk Correlations Physics Working Group EVO meeting

2008-10-29 11:00
2008-10-29 12:30
Etc/GMT-5
Wednesday, 29 October 2008
EVO, STAR Community, at 15:00 (GMT), duration : 01:30
Meeting is locked (you cannot add new talks anymore)

Please upload agenda items, or links to agenda items

S&C Infrastructure Servers

 

2008.10.27 SMD-based shower shape scaling: 25 strips cluster energy, raw vs. data-driven MC

Ilya Selyuzhenkov October 27, 2008

Data sets:

Draft STAR note

Draft STAR note

STAR database inrastructure improvements proposal

 

STAR database improvements proposal

Comparison of spectra run 3 vs run 8

 Below is an attempt to look at spectra in run 8 vs run 3 d+Au.

nonphotonic electrons in the Endcap EMC

nonphotonic electrons in the Endcap EMC

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

2008-10-22 10:00
2008-10-22 11:00
Etc/GMT-7
Wednesday, 22 October 2008
BNL, 50-I-189, at 14:00 (GMT), duration : 01:00

Conference Phone Number: 510 486 7333

   Time:  10 - 11 am EDT

 * --===================================--*

  Agenda:

    0) Joule targets for FY09 - Bill

    1) QM09 speaker discussions - Nu

    2) STAR computing plan - Jerome

* --===================================--*

    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:

conversion tomagraphy

conversion tomagraphy

2008 (FY09) R&D

FY09 R&D requests:

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.

2008.10.15 Purity vs. efficiency from gamma-filtered events: R_cluster > 0.9 vs. R_cluster > 0.98

Ilya Selyuzhenkov October 15, 2008

Data sets:

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:

2008.10.13 Jet trees for Michael's gamma filtered events

Ilya Selyuzhenkov October 13, 2008

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