Difference between revisions of "AW Singles Prob Y88 2015"
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− | <math>N(\frac{1836}{898}) =\frac{\frac{ UN(1836)}{.31}}{ \frac{UN(898)}{.78}}=\frac{5}{2} \frac{UN(1836)}{ UN(898)}=1 =</math> Ratio | + | <math>N\left (\frac{1836}{898}\right ) =\frac{\frac{ UN(1836)}{.31}}{ \frac{UN(898)}{.78}}=\frac{5}{2} \frac{UN(1836)}{ UN(898)}=1 =</math> Ratio |
Revision as of 18:27, 3 February 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.
Ratio
UCR ratio before efficiency correction
Days | (898 keV) Integral Raw | (1836 keV) Integral Raw | UCR | (898 keV) Integral Eff Cor | (1836 keV) Integral Eff Cor | Ratio | |
108 | 1.01 | 1.364 Media:Run7022_898_raw.png | 0.8414 Media:Run7022_1836_raw1.png | 0.0480.62 | 174.2 | 13.24269.8 | 30.911.55 |
159 | 1.49 | 0.8697 Media:Run7107_898_raw.png | 0.5015 Media:Run7107_1836_raw.png | 0.0420.58 | 111.07 | 9.753160.8 | 20.91.45 |
229 | 2.15 | 0.4733Media:Run7203_898_raw_ratio3.png | 0.2822 Media:Run7203_1836_raw_nocut.png | 0.0590.60 | 60.45 | 8.27290.48 | 20.951.50 |
245 | 2.30 | 0.5807 Media:Run7235_898_raw.png | 0.2449 Media:Run7235_1836_raw.png | 0.0320.42 | 74.16 | 7.71878.52 | 12.891.06 |
What is the background contribution to the above rates
Efficiency corrected plot of the two activities as a function of days