The STAR experiment

Here I give rough estimates for the radiation we can expect for the inner ring on the currently considered forward TOF rings. Rates are taken from run 7.

To perform a check on the BEMC calibration for run 7, I began by looking over the electrons from the StGamma production. 

Following the analysis in 2006 TPC Drift Velocity Investigation we did a test production with the new interpolated DV values.  Here's a plot as the magnitude of the global DCA for primary tracks from run 7142036 (pt>2,

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This page summarizes the time-dependent L2 configuration in 2006.

    Another simple algorithm would be to calculate the distance between the highest energy strip and the mean of the distribution (from here I'll refer to this as MMM for "mode min

L2gamma2008 trigger strawman

10/23/2007

    Our second attempt at utilizing the SMD information for direct photon/background discrimination this time using the popular variable

Problem:

Test Blog Jan