Difference between revisions of "AW Singles Prob Y88 2015"

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| Days ||<math>T_{1/2}</math> ||  (898 keV) Integral Raw||  (1836 keV) Integral Raw||  Ratio || (898 keV) Integral Eff Cor||  (1836 keV) Integral Eff Cor || Ratio
 
| Days ||<math>T_{1/2}</math> ||  (898 keV) Integral Raw||  (1836 keV) Integral Raw||  Ratio || (898 keV) Integral Eff Cor||  (1836 keV) Integral Eff Cor || Ratio
 
|-
 
|-
| 108 ||  1.01 ||1.364 <math>\pm 0.062 [[File:Run7022_898_raw.png]]</math>
+
| 108 ||  1.01 ||1.364 <math>\pm 0.062 [[Media:Run7022_898_raw.png]] </math>
 
|-
 
|-
 
| 159 ||  1.49 ||  0.8697  <math>\pm 0.055  </math>
 
| 159 ||  1.49 ||  0.8697  <math>\pm 0.055  </math>

Revision as of 18:30, 27 January 2015

Problem description:

The singles spectra production for the initial Y-88 activity is off by a factor of 2.
Right now the high energy line is a factor of 2 higher.



Days [math]T_{1/2}[/math] (898 keV) Integral Raw (1836 keV) Integral Raw Ratio (898 keV) Integral Eff Cor (1836 keV) Integral Eff Cor Ratio
108 1.01 1.364 [math]\pm 0.062 [[Media:Run7022_898_raw.png]] [/math]
159 1.49 0.8697 [math]\pm 0.055 [/math]
229 2.15 0.4733[math]\pm 0.058 [/math]
245 2.30 0.5807 [math]\pm 0.049 [/math]


A_W_thesis#Final_problems_to_sort_out