K40 Background Simulations for the Seawiet OM
K40 Background Simulations for the Seawiet OM
K40 Background Simulations for the Seawiet OM
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Summary and Outlook<br />
most correlated coincidences<br />
• originate from within 5 m from <strong>the</strong> <strong>OM</strong>, <strong>the</strong>re<strong>for</strong>e<br />
absorption length has little effect<br />
• are distributed to two or more PMTs<br />
• occur in PMTs next to each o<strong>the</strong>r<br />
calibration opportunities<br />
from <strong>K40</strong> coincidences:<br />
• s.p.e. response<br />
• time calibration<br />
(under investigation)
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