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Search for Dark Matter Captured in the Sun with ... - KICP Workshops

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The observed angle to <strong>the</strong><br />

<strong>Sun</strong> is fitted <strong>with</strong> signal and<br />

background pdf:s<br />

Maximum llh-analysis<br />

How many signal events can be<br />

consistent <strong>with</strong> <strong>the</strong> observation?<br />

Evaluate shape fit <strong>with</strong> log−<br />

likelihood rank (Feldman-Cous<strong>in</strong>s)<br />

to construct confidence regions<br />

<strong>for</strong> <strong>the</strong> number of signal events μs<br />

where L is <strong>the</strong> pdf product over <strong>the</strong><br />

f<strong>in</strong>al sample<br />

23/07/12 Matthias Dann<strong>in</strong>ger IDM 2012<br />

background expectation from data<br />

Angle between event track and direction<br />

from <strong>the</strong> <strong>Sun</strong><br />

observation<br />

signal simulation (e.g. 1000 GeV)<br />

10

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