Time	Talk	Presenter
13:00	Andre´s abstract for Hard Probes ( 00:10 ) 0 files
13:10	Xiaoyan´s abstract for Hard Probes ( 00:10 ) 0 files
13:20	Jaro´s abstract for Hard Probes ( 00:10 ) 0 files

Time	Talk	Presenter
17:00	SQM JPsi talk ( 00:15 ) 0 files	Johan

The following steps explain how to perform the calibrations of the SpaceCharge and GridLeak database entries.

Comparison of RICH scalers

The low energy CuCu runs are a difficult spot for E-by-E SpaceCharge calibrations: the time-averaged multiplicity of recorded tracks traversing the TPC is unlikely

This is an highlight of the HSI features. Please, visit the HSI Home Page for more information.

To use htar within the HPSS environment, users are required to have the valid Kerberos credentials.

The following is the man page of how to use htar.

   
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In an effort to better understand the future of the TPC in the high luminosity regime, several meetings were held and efforts carried through.

Present at the meeting(s) were: myself (Jerome Lauret), Alexei Lebedev, Yuri Fisyak, Jim Thomas, Howard Wiemann, Blair Stringfellow, Tonko Ljubicic, Gene van Buren, Nikolai Smirnof, Wayne Betts (If I forgot anyone, let me know).

For users

QuickStart.pdf is for Globus version 1.1.3 / 1.1.4 .

Using tracks fit with SVT points plus a primary vertex alone, we can self-align the SVT using residuals to the fits. This document explains how this can be done, but only works for the situation in which the SVT is already rather well aligned, and only small scale alignment calibration remains.