FGT disks (Delivery, July 28, 2011)

mass dependence of relative beam intensity (modified)

1. As was suggested, the cuts for pion candidates need to be studied when examine the effect of beam intensity and LED corrections within a fill.

Comparison of 2009 pp500GeV data to 2006 pp200GeV MC

Run 9 200GeV Dijet High Pt Tail Investigation

Here I detail my exploration of the high pt tail seen in the pr

2011 Spin QA: Transverse Running

2011 Spin QA: Transverse Running

 

Thoughts on implementing y2012 in AgML and integrating with STARSIM framework

1. The current starsim geometry interface should be preserved.  Users should still be able to instantiate geometry using

mass dependence of relative beam intensity

In order to see if the pion mass has a dependence on beam intensity, not just run number (or time). I estimated the beam intensity for each run in 2 fills.

AOB

Speaker : All ( All )


Talk time : 12:55, Duration : 00:05

TPC anode voltages work overview

Speaker : Yan Yang ( Wuhan )


Talk time : 12:35, Duration : 00:20

Status on vertex finding ranking issues

Speaker : Anthony Kesich ( UC-Davis )


Talk time : 12:20, Duration : 00:15

Status on Stv development

Speaker : Victor Perevoztchikov ( BNL )


Talk time : 12:00, Duration : 00:20

Software and Computing Meeting

2011-07-27 12:00
2011-07-27 13:00
America/New York
Wednesday, 27 July 2011
1-189, EVO, at 16:00 (GMT), duration : 01:00
TimeTalkPresenter
12:00Status on Stv development ( 00:20 ) 1 fileVictor Perevoztchikov (BNL)
12:20Status on vertex finding ranking issues ( 00:15 ) 1 fileAnthony Kesich (UC-Davis)
12:35TPC anode voltages work overview ( 00:20 ) 1 fileYan Yang (Wuhan)
12:55AOB ( 00:05 ) 0 filesAll (All)

Christie's Operations Documents Distribution Page.

Under:

Bug in PHMDGEO

There is an (undocumented) limitation in the length of lines in an AgSTAR geometry file.  Any line longer than 122 characters is trucacted at 122 characters.  Violation of this limit is f

Shower Shape Studies from Run11 data: Progress Report 2

This is an update (second) on the current progress of studying shower shapes in Run11 data. Some detail of how the study is being done (i.e.

FMS Meeting - 7-25-2011

I've updated the gain correction dependent plots to include more information about the cell and adjacent cells while the gain correction is changed. 

test/Seema 3-Gauss fit param vs. preshw bin and ESMD u-V

I took the 3-Gaussian ESMD shower shape fit values from the spread sheets attached to Seema's blog:

Update on LED corrections

1.

Sector dependent shower shapes sorted into different preshower bins - Triple Gaussian Fits (Version 2)

 Transverse Shower Profile Distributions 

 

Run 9 200GeV Dijet Stats & QA: Test 2

I have rerun my QA, kinematic, false asymmetry, and dijet ALL statistics analysis originally seen

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