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calculation of correction factor to kt with STAR simulated datasets for dijets.
Updated on Mon, 2009-09-21 01:27. Originally created by mriganka on 2009-09-10 14:53.Di-jet cross section from the page :
Rough cut of EEMC SMD spacer geometry
The SMD spacer is added to the EEMC geometry, as well as material in the front and back of each SMD plane.
Ws at STAR Run 9 - spin PWG presentation
Updated on Mon, 2009-09-28 14:23. Originally created by balewski on 2009-09-10 08:51.
Proceedings EPS 2009 STAR FGT Project
Updated on Wed, 2009-09-09 20:28. Originally created by surrow on 2009-09-09 20:28.2005 Dijet Cross Section Preliminary Presentation
Updated on Thu, 2009-09-17 10:49. Originally created by mattheww on 2009-09-09 13:17.Attached is my preliminary presentation for the 2005 Dijet Cross Section to be shown on Thursday, September 10, 2009.
Comparing data etas to simulated etas
In the attached plots I'm comparing the etas I have found in different sectors in data to a single particle eta simulation in MC which has been put through the same analysis code. I throw the
UPC analysis
This is my first attempt to use a blog. I attach a ppt file with a report on analysis of muDST from run07 UPC triggers
The BBC vernier scan calculation is really clean
Updated on Tue, 2009-09-08 16:00. Originally created by rcorliss on 2009-09-08 16:00.I've found one of the problems in the code, and am now off by a (measly) two or so orders of magnitude.
W-Background Estimation based on Run 9 pp500 data
I'm using Jan's Algo ver 4.1 with a few modifications to look into the idea Scott suggested of sorting events by placing conditions on the away side to get an estimate of the background. Here
vernier scan timing from Angelika
Updated on Tue, 2009-09-08 15:42. Originally created by rcorliss on 2009-09-08 15:42.The following are the raw times Angelika gave me for the vernier scans, along with her verbatim description of the same (lifted from emails):