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EVO

This section contains information about using EVO for STAR meetings.

06 comparison of BTOW status bits L2ped vs. L2W , pp 500 (jan)

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 Comparison of BTOW status tables generated based on minB spectra collected by L2ped ( conventional method) vs.

200904

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Collaboration Meeting Presentation and wrap up.

 Attached is the presentation I gave at the collaboration meeting in late March.

01 Status of BSMDE,P at the end of pp 500 GeV run, April of 2009

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Summary of BSMD performance on April 6.

QA Reference for Trigger Specific Histograms - Run 9

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STAR Offline QA Shift Histogram Description - Run 9

Note:  Not all reference plots may be ideal, be sure to ca

QA Reference for General Histograms - Run 9

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STAR Offline QA Shift Histogram Description - Run 9

Fast Offline QA Histogram References and Descriptions

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03 periodic summary of all acquired events

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att 1) all W-events for ~300K from days 76-89

att 2) one fill from day 83, 34K W-events, I think BPRS peds were not subtracted for some runs, page 7 

Calibration Uncertainty Calculation

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Summary:

Integral Delta G Study

 Using Werner's code I calculated A_LL for pi0 production over my eta range for 15 different integral values of Delta G.

02 QA of TPC tracks

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 Daq files with W events were reco w/ BFC "pp2009a ITTF BEmcChkStat QAalltrigs btofDat Corr3  beamLine -VFMinuit  VFPPVnoCTB -dstout -evout"

Event cuts:

Run 9: pp500 Low Luminosity Fill

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 The low luminosity fill was taken using runs 10083130, 133, 139, and 143, with BBC coincidence rates of ~50 kHz, using the BBCMB trigger.

y2005gStar

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y2008aTpce

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y2008aStar

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y2009Tpce

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y2009Star

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01 BPRS live channels on day 82, pp 500 data

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Status of BPRS live channels on March 23, 2009, pp 500 data.

Input: 32K events accepted by L2W algo, from 31 runs taken on day 81 & 82.

y2008yfTpce

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