This thesis describes the results of a chi2 analysis designed to reject events occurring near detector surfaces. Because no WIMP signal was observed, separate limits using the germanium and silicon detectors are set on the WIMP cross section under standard astrophysical assumptions.crate slot number of the board for which the command was issued. 3.4.3 Veto Electronics Ia#39;ll begin describing ... NIM Crates Amp/Fan-Out Boards Amplified/ Stretched Veto Signals Veto Signals Scaler 131 3.4. DATA ACQUISITION HARDWAREanbsp;...
|Title||:||Results from the Cryogenic Dark Matter Search Using a Chi Squared Analysis|
|Publisher||:||ProQuest - 2007|