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The SVT Group pages are available on the old Web site.

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Welcome to the STAR sub-system page. The menu displays all major sub-systems in the STAR setup.

Proton-lambda residual correlations in proton-proton- update

Reference

Speaker : Hania Gos ( Warsaw University of Technology, SUBATECH )


Talk time : 19:00, Duration : 00:10

GL_pp400_X30_High

GL_pp400_X30_High

GridLeak plot for pp400 data with 30% above standard pp200 corrections, high luminosities

GL_pp400_X17_Lowest

GL_pp400_X17_Lowest

GridLeak plot for pp400 data with standard pp200 corrections, lowest luminosities

GL_pp400_X17_High

GL_pp400_X17_High

GridLeak plot for pp400 data with calibrated corrections, high luminosities

GL_pp400_STD_High

GL_pp400_STD_High

GridLeak plot for pp400 data with standard pp200 corrections, high luminosities

GL_pp400_NONE_Low

GridLeak plot for pp400 data with no correction, low luminosities

GL_pp400_NONE_High

GL_pp400_NONE_High

GridLeak plot for pp400 data with no correction, high luminosities

AOB

Reference

Speaker : All


Talk time : 12:40, Duration : 00:10

GridLeak plots

Looking at the residuals (GridLeak plots), I can see that things are similar to pp200, witth what appears to be an offset in GridLeak distortion at all z (our current understanding of the distortion has it go to zero at the ground planes, |z| = 208 cm). I include here three plots of GridLeak distortion residuals from tracks for high luminosity pp400 data (runs 6154024-6154031, bbce+bbcw > 2e5):

Production update

Reference

Speaker : Lidia Didenko ( BNL )


Talk time : 12:30, Duration : 00:10

MC comparison TPT/ITTF for Au+Au and Cu+Cu

Reference

Speaker : Yuri Fisyak ( BNL )


Talk time : 12:15, Duration : 00:15

STAR Upgrades Meeting

-00-00
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from Thursday, 1 January 1970 to Thursday, 1 January 1970
Conference duration: 1 day

Upgrades meeting

Calibration status for Cu+Cu and p+p 400 GeV

Reference

Speaker : Gene Van Buren ( BNL )


Talk time : 12:00, Duration : 00:15
For this presentation, please see the page pp400 (2005).

December 2005 STAR Analysis Meeting

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from Thursday, 1 January 1970 to Thursday, 1 January 1970
Conference duration: 1 day

Biannual STAR Analysis Meeting