mktxt2005.txt

Under:
#!/bin/csh

set sdir = ./StarDb/Calibrations/rhic
set tdir = ./txt
set files = `ls -1 $sdir/*.C`
set vs = (x0 err_x0 y0 err_y0 dxdz err_dxdz dydz err_dydz stats)
set len = 0
 

queryNevtsPerRun.txt

Under:
-- N evts per run, where N is the numerator at the end of the last line

select floor(bi.blueFillNumber) as fill,
sum(ts.numberOfEvents/ds.numberOfFiles) as gdEvtPerFile,
 

Run 5

2005 Beamline Calibration

Information about how this calibration is done, and links to other years, can be found You do not have access to view this node.

Run 6 (pp)

 

Run 4 (pp)

 

Run 2 (200 GeV pp)

Finding primary vertex seeds

What is done to find the seeds

Pass 1

In this pass, the seed finding was done on a per-run basis.

Run 3 (200 GeV dAu and pp)

 

Is the ridge formed by alignment of jet propagation and medium flow direction?

Speaker : Joshua Konzer ( Purdue )


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

Addressing the physics of the ridge by 2- and 3-particle correlations at STAR

Speaker : Pawan Netrakanti ( Purdue )


Talk time : 11:45, Duration : 00:45

Looking forward for Color Glass Condensate signatures with STAR STAR

Speaker : Ermes Braidot ( Utrecht )


Talk time : 11:00, Duration : 00:45

Jet-like correlation Physics Working Group

TimeTalkPresenter
11:00Looking forward for Color Glass Condensate signatures with STAR STAR ( 00:45 ) 0 filesErmes Braidot (Utrecht)
11:45Addressing the physics of the ridge by 2- and 3-particle correlations at STAR ( 00:45 ) 1 filePawan Netrakanti (Purdue)
12:30Is the ridge formed by alignment of jet propagation and medium flow direction? ( 00:30 ) 0 filesJoshua Konzer (Purdue)

Jet reconstruciton

Jet reconstruction

Di-Hadron fragmentation function in p+p collisions at 200 GeV at STAR

Initial state nuclear effects for jet production measured in 200 GeV d+Au collisions by STAR

Speaker : Jan Kapitan ( Czech NPI )


Talk time : 11:15, Duration : 00:30

Decomposing p+p Events at 200 GeV with STAR

Gamma triggered 2+1 correlation