Difference between revisions of "Elong-13-06-03"

From HallCWiki
Jump to navigationJump to search
Line 4: Line 4:
  
 
::{| class="wikitable" style="text-align:center; border-collapse:collapse;" border="1"
 
::{| class="wikitable" style="text-align:center; border-collapse:collapse;" border="1"
| style="width: 200px;" | <math>x_{\mathrm{Spectrometer}}</math> || style="width: 200px;" | <math>dA_{zz}^{drift}(x_{spec})</math>
+
| style="width: 200px;" | <math>x_{\mathrm{Spectrometer}}</math> || style="width: 200px;" | <math>dA_{zz}^{drift}</math>
 
|-  
 
|-  
 
| 0.15 || 0.0046
 
| 0.15 || 0.0046

Revision as of 16:45, 3 June 2013

Including Drift by Bin

Dustin's work on the drift has given a different value depending on the spectrometer setting, which are shown in the table below.

<math>x_{\mathrm{Spectrometer}}</math> <math>dA_{zz}^{drift}</math>
0.15 0.0046
0.30 0.0037
0.45 0.0028
0.55 0.0021

For the plots using the spectrometer settings as bins, where <math>A_{zz}</math> and <math>b_1</math> are in blue and red, these are included as an additional systematic uncertainty.

For the rebinned plots, where <math>A_{zz}</math> and <math>b_1</math> are in pink, each of the drift uncertainties are added as a weighted average. The weights are the number of events that each spectrometer contributes to the rebinned statistics.

That's to say,

<math>dA_{zz}^{Ave. Drift} = \frac{\sum \left( dA_{zz}^{drift}N_{Spec} \right)}{N_{Total}}</math>

where <math>dA_{zz}^{drift}</math> is shown in the table above for each spectrometer setting, <math>N_{Spec}</math> is the number of events from a particular spectrometer setting that go into this x bin, and <math>N_{Total}</math> is the total number of events, from all spectrometer settings, that go into this x bin.

Conservative Estimates

If we apply these with a conservative estimate, with <math>P_{zz}=20\%</math> and <math>dA_{zz}^{(Rel. Sys)} = 12\%</math>, we can estimate both the full spectrometer bins:

2013-06-03-spec-Pzz-20.png

We can then use a weighted average for <math>dA_{zz}^{drift}</math>, where the weights are number of events that each spectrometer setting contributes to a particular <math>x</math> bin. The rebinned estimate is then:

2013-06-03-Pzz-20.png

Same as above, but if we split the systematic uncertainty into bars, we get:

2013-06-03-Pzz-20-bar.png

Optimistic Estimates

If we apply these with an optimistic estimate, with <math>P_{zz}=40\%</math> and <math>dA_{zz}^{(Rel. Sys)} = 9\%</math>, we can estimate both the full spectrometer bins:

2013-06-03-spec-Pzz-40.png

We can then use a weighted average for <math>dA_{zz}^{drift}</math>, where the weights are number of events that each spectrometer setting contributes to a particular <math>x</math> bin. The rebinned estimate is then:

2013-06-03-Pzz-40.png

Same as above, but if we split the systematic uncertainty into bars, we get:

2013-06-03-Pzz-40-bar.png

--E. Long 20:58, 3 June 2013 (UTC)