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G060065-00

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Coherent network analysis technique for discriminating GW bursts from instrumental noise Patrick Sutton (CIT) in collaboration with Shourov Chatterji, Albert Lazzarini, Leo Stein (CIT), Antony Searle (ANU), Massimo Tinto (CIT/JPL)
Motivation ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Null Streams whitened noise noise-weighted antenna response varies with sky position, frequency ,[object Object],[object Object],[object Object],[object Object]
GWBs vs Glitches ,[object Object],[object Object],[object Object],[object Object]
Sky Maps: Null Energy / DOF Glitch GWB ,[object Object],[object Object],[object Object]
Sky Maps: Incoherent Energy / DOF Glitch GWB ,[object Object],[object Object]
Sky Maps: ( E null – E inc ) / DOF Glitch GWB ,[object Object],[object Object],source location
GWB vs. Glitch Correlated energy Correlated energy ,[object Object],[object Object],[object Object],GWB has off- diagonal points Glitch falls on diagonal
Measures of Correlation ,[object Object],[object Object],[object Object]
New Since GWDAW ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Waveforms: 3 DFMs (supernovae) ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
GWBS vs. Glitches: Most Correlated Positions ,[object Object],[object Object],[object Object],10  rms = 100 50 5 20
ROC: Distinguishing GWBs from Glitches ,[object Object],[object Object]
E null only ,[object Object],[object Object]
Energy Difference: E null - E inc ,[object Object]
E null only ,[object Object],[object Object],[object Object]
Using only Null Energy (GT) ,[object Object]
Conclusions ,[object Object],[object Object],[object Object],[object Object],[object Object]
To Do List ,[object Object],[object Object],[object Object],[object Object],[object Object]

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G060065-00

  • 1. Coherent network analysis technique for discriminating GW bursts from instrumental noise Patrick Sutton (CIT) in collaboration with Shourov Chatterji, Albert Lazzarini, Leo Stein (CIT), Antony Searle (ANU), Massimo Tinto (CIT/JPL)
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