SSD status
Updated on Mon, 2012-10-15 09:54. Originally created by videbaks on 2012-09-29 15:56.IST status
Updated on Mon, 2012-10-15 09:51. Originally created by videbaks on 2012-09-29 15:56.Reference
Speaker : Gerrit van Nieuwenhuizen II
Talk time : 10:40, Duration : 00:30
PXL status
Updated on Mon, 2012-10-15 09:52. Originally created by videbaks on 2012-09-29 15:55.HFT overview
Updated on Sat, 2012-09-29 15:49. Originally created by videbaks on 2012-09-29 15:49.HFT F2F
Updated on Sat, 2012-09-29 15:45. Originally created by videbaks on 2012-09-29 15:45.LBL , at 13:30 (GMT), duration : 00:00
Time | Talk | Presenter |
---|---|---|
09:30 | HFT overview ( 00:40 ) 1 file | F.Videbaek (BNL) |
10:10 | PXL status ( 00:30 ) 1 file | L.eo Greiner |
10:40 | IST status ( 00:30 ) 1 file | Gerrit van Nieuwenhuizen II |
11:10 | SSD status ( 00:20 ) 1 file | Jim Thomas |
11:30 | Cost and Schedule ( 00:20 ) 1 file | Sarah Morgan |
13:00 | Software plans discussion ( 00:20 ) 3 files | Spiros Margetis |
13:20 | Integration ( 00:20 ) 1 file | R.Sharma |
13:40 | Global structures ( 00:20 ) 1 file | Eric Anderssen |
Effect of beam dump through a 1% interaction length target placed at z=-2m
amplitude vs adc
Here I show the sum of time bin ADCs vs the amplitude fit paramater for each apv on disc 6 quad 1.
strip-by-strip fit parameter distributions
I'm looking at strip-by-strip fit parameter distributions for the P-layer. I looked at 8 strips with the highest counts in disc 6 quad 1 apv 14. In each figure, the plot on the top-left
timebin fits for residuals
I tried to use timebin fits to get to the residuals.
In short, it didn't improve things.
The first issue is the stability of the fiits for low amplitudes.
IST : update on geometry
Updated on Fri, 2012-09-28 12:19 by margetis. Originally created by bouchet on 2012-09-28 10:32.Run-11 Transverse Jets: Collins and Sivers (Run List Part I)
Update: September 30, 2012
It was pointed out to me that I labeled the figures in terms of θjet. This is a mistake.
DIGMAPS and StPixelFastSimMaker
Updated on Thu, 2012-09-27 23:45. Originally created by mstftsm on 2012-09-27 23:45.Vertex Z Acc/Rej
It was suggested to try weighting the Pythia sample in order to have it match the vertex distribution.
IU and TSIU Algos: Procedural Comparison
IU Algorithm
- Initialize "seed floors" to zero
- Starting with strip 3 and going until 3 before the last strip
Three particle correlations
Jim Thomas and I have analyzed various three particle correlations of the form cos(n*phi_i + m*phi_j - (n+m)*phi_k). We intend to publish the results ASAP.
Background Asymmetries
Contained herein are the background asymetries for the longitudinal single and double spin asymetry for 2006 inclusive pi0s in the EEMC.
Residuals, cosmic run 40-45 with Gaussian fits
Residuals with gaussian fits over strips.
To make sure that one actually fit a gaussian I extended 1 and 2 strip wide clusters to 3 strips