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S.Klimenko, March 2003, LSC Burst Analysis in Wavelet Domain for multiple interferometers LIGO-G030132-00-Z Sergey Klimenko University of Florida l Analysis strategy l Data analysis pipeline WaveMon veto generator (S.Klimenko, see LIGO note G020383-00-Z) WaveBurst event generator (S.Klimenko, I.Yakushin) l Analysis algorithms l Some results for S1 l Summary & Plans
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S.Klimenko, March 2003, LSC Analysis strategy l Triggers are generated independent for each IFO l GW candidates are generated on the final coincidence step GW events coincidence VETO ETG: tfcluster, slope, power VTG: glitch monitors ifo1 auxiliary channels VETO ETG: tfcluster, slope, power VTG: glitch monitors Ifo1,… auxiliary channels
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S.Klimenko, March 2003, LSC event trigger generators l pixels produced by artifacts are clustering together - very powerful idea behind the Time-Frequency cluster analysis l use coincidence to enhances it. l coincidence is used before the events are generated approach often used in HEP. data conditioning: wavelet transform, rank statistics, pixel selection channel 1 data conditioning: wavelet transform, rank statistics, pixel selection channel 2,… “coincidence” event generation event generation WaveBurst/WaveMon data conditioning: Fourier transform, Gaussian statistics, pixel selection channel 1 event generation TFCLUSTER
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S.Klimenko, March 2003, LSC Wavelet Transform l Optimize search by selecting wavelet type & decomposition tree l detail coefficients d i represent data in different frequency bands df = f/2, f/4, f/8, ….. - dyadic, df = f/n, - linear basis wavelet transform tree d0d0 d1d1 d2d2 a db8
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S.Klimenko, March 2003, LSC wavelet time-scale(frequency) plane l For short (therefore broadband) bursts dyadic WT should be good. l For long signals, like inspirals, binary WT could be optimal l Several wavelet transforms are implemented in the datacondAPI l Currently used in WaveBurst: interpolating bi-orthogonal, Daubechies, Simlets binary wavelet tree (linear frequency scale)
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S.Klimenko, March 2003, LSC Percentile Transform l given a sample with amplitude A, define its percentile amplitude as a=1/f, where f is fraction of samples in the population with absolute value of amplitude greater then | A| l Equivalent to calculation of rank statistics non-parametric l percentile amplitude distribution function: P(a)=1/a 2 the same for all wavelet layers
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S.Klimenko, March 2003, LSC raw percentile TF plots H2:LSC-AS_Q H2:IOO-MC_F
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S.Klimenko, March 2003, LSC 10% H2:LSC-AS_Q 224-240 Hz 10% Percentile Thresholding Rule l threshold on percentile amplitude l select a certain fraction of samples (set T-F occupancy) l don’t care about the data distribution function l one possible way of “de-noising of wavelet data”
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S.Klimenko, March 2003, LSC Coincidence Rules accept reject l Given local occupancy O i (t,f) in each channel, after coincidence the cluster occupancy is l For strict coincidence O i (t,f) = p 2 for random pixels produced by noise. for example if p=0.1, average occupancy after coincidence is 0.01 l WaveBurst can use various coincidence policies allows customization of the pipeline for specific burst searches.
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S.Klimenko, March 2003, LSC strict coincidence l coincidence TF plot for LSC-AS_Q && IOO-MC_F l coincidence allows set a low threshold at the previous (thresholding) step “build” clusters with known false alarm rate, determined by random clustering of pixels
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S.Klimenko, March 2003, LSC Cluster Analysis Cluster Parameters size – number of pixels in the core volume – total number of pixels density – size/volume amplitude – maximum amplitude power - wavelet amplitude/w50 energy - power x size asymmetry – (#positive - #negative)/size likelihood – log( A i ) neighbors – total number of neighbors frequency - core minimal frequency [Hz] band - frequency band of the core [Hz] time - GPS time of the core beginning interval - core duration in time [sec] cluster core positive negative Cluster halo cluster – T-F plot area with high occupancy
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S.Klimenko, March 2003, LSC ‘orthogonal’ data sets l WaveMon/WaveBurst generate clusters of three types: candidate clusters potential GW bursts off-time clusters (due to random coincidence of glitches) veto tuning “false alarm” clusters (due to random clustering of noise) threshold settings quiet channel hot channel WaveMon rates for coincidence with H2:LSC-AS_Q S1 data blue – candidates red – off-time green - random
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S.Klimenko, March 2003, LSC selection cuts: cluster likelihood l L threshold can be set a priori based on the false alarm rate does not need tuning perfect for real time processing Only L threshold is applied at run time ETG output rate ~0.2Hz SG strain=5e-18 100-2000 Hz
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S.Klimenko, March 2003, LSC selection cuts: cluster “energy” For Gaussian noise E= 2 l Energy cut is set based on the false alarm rate and it is used for post-processing event selection w i – wavelet amplitude w 0 – distribution median w 50 – median of |w i -w 0 | S1 playground Software injections strain=5e-18
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S.Klimenko, March 2003, LSC VETO l After applying selection cut, remaining events are suppose to be removed with vetoes l Veto events can be generated by DMT monitors and by ETGs itself. l Off-time data set (red dots) is used for selection of effective veto channels nothing to veto for S1 playground data, except for frequency band<150Hz But veto will be very important for large data sets work in progress on optimization of veto strategy no whitening
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S.Klimenko, March 2003, LSC Other issues l Simulation study using injected bursts: pipeline consistency check. efficiency study for different coincidence policies using bursts injected randomly in time and with random delay between detectors. l X-correlation between burst candidates found in two detectors. Could be significant enhancement of the search pipeline. (see Malik’s talk)
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S.Klimenko, March 2003, LSC Conclusion & Plans l WaveBurst ETG produces GW burst candidates for a coincidence of two detectors uses non-parametric statistics allows a priori threshold settings for the on-line operation. produce event triggers with known false alarm rate l WaveMon monitors the detector glitch performance Can help identify the source of glitches in the GW channel by looking at frequency content and correlation with auxiliary channels produces veto triggers l Plans Use S1 as a playground for WaveBurst pipeline. Process S2 Preparations for S3
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