1. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) Data conditioning and veto for TAMA burst analysis Masaki Ando and Koji Ishidoshiro (Department of Physics, University of Tokyo) and the TAMA Collaboration

2. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 2 Introduction (1) - Veto analysis - Veto analysis by monitor signals GW detector is sensitive to external disturbances as well as real GWs Reject fake events using monitor signals recorded together with the main output of the detector Main outputMonitor signals Data conditioning (Whitening, freq.-band selection, Line removal) Burst-event extraction (Burst filter: excess-power filter) Coincidence analysis GW candidatesFake events No Yes Systematic survey of all monitor channels Fake reduction even without understandings of noise mechanisms

3. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 3 Introduction (2) - TAMA DT9 data - TAMA data acquisition and analysis system Used data in this work: TAMA DT9 (Dec. 2003 – Jan. 2004) 200 hours of data (HDAQ 8ch, MDAQ 64ch)

4. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 4 Data Conditioning

5. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 5 Data conditioning (1) - Quality of data from detectors - Data conditioning ‘ideal’ data (predictable behavior known statistics) Stationary noise White noise Real data from detectors Non stationary behavior Drift of noise level Sudden excitations Frequency dependence Sensitivity degradation in high and low frequencies Line noises DT9 DT8 DT6 Data conditioning

6. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 6 Data conditioning (2) - TAMA conditioning filter - Data conditioning for TAMA burst analyses Normalization of the data by averaged nose level  Remove time and frequency dependence Line removal Select frequency band to be analyzed In addition … Calibration : Convert v (t) to h (t) Resampling : Data compression Requirements Small loss in signal power Keep GW waveform

7. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 7 Data conditioning (3) - Data flow - Data conditioning by FFT-IFFT Frequency selection, Whitening/Calibration, Resampling Fourier transform 72sec data Frequency-band selection Overwrite ‘0’ for unnecessary frequencies Outside of the observation band AC line freq., Violin-mode freq. Calibration peak Whitening Normalize by avg. spec. Calibration Convert to h(f) Raw time- series data 20kHz samp. Inverse Fourier transform Only below 5kHz Whitened time- series data 5kHz samp. Calibrated time- series data 5kHz samp.

8. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 8 Data conditioning (4) - Results of conditioning - Whitened data Without resamp. 5kHz resamp. Zoom Spectrum  Whitened Time-series data  Waveform is maintained with resampling

9. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 9 Data conditioning (5) - Calibrated spectrum - Calibrated data Blue: FFT of raw data  calib. Red: Conditioned data Power spectrum of conditioned time-series data and calibrated spectrum of original data

10. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 10 Event extraction

11. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 11 Event extraction (1) - Excess power filter - Burst event trigger Excess-power filter Evaluate power in given time-frequency windows  Extract non-stationary events Data conditioning time-series data in a given frequency band Calculate power in a given time window Power in a given time-frequency window  SNR Threshold, Clustering  Burst events Free selection of time-frequency window Previous works… Spectrogram  Averaged power Time-frequency resolution were limited by FFT length

12. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 12 Veto analysis

13. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 13 Veto analysis (1) - Concept - Coincidence analysis External disturbances tend to appear in some monitor signals  Reject fake events Burst events Coincidence  Reject GW candidate Threshold Main output (SNR) Monitor (SNR) Time * Simulated data

14. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 14 Veto analysis (2) - Parameter optimization - Parameter optimization Analysis parameters Time-frequency window Threshold Signals to be used for veto Optimized to have… High fake-rejection efficiency Low accidental coincidence Time-frequency window: Highest coincidence rate selected from 50 (18) time-frequency combinations Threshold for monitor signals: Accidental ~ 0.1% Accidental coincidence: estimated by 1-min.time-shifted data Coincidence ratio Accidental coincidence Coincidence Playground data (~10%) are used for this optimization 0.1% SNR Threshold (monitor signal)

15. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 15 Veto analysis (3) - Signal selection - Signal selection Even with small accidental rejection prob. (~0.1%) for each, many (~100) monitor signals may lose large amount of data Select signals to be used for veto Classify by the coincidence rate… <0.5 %  Do not use for veto 0.5 - 2 %  Use for veto > 2%  Intensive veto with lower threshold: accidental ~ 0.5% Intensive fake-rejection with some monitor signals with strong correlations with the main signal Re-optimize the threshold HDAQ: 3 signals Rec. Pow., L+ FB, Dark Pow. MDAQ: 9 signals l- Err., l- FB, l+ Err., l+ FB, Bright Pow, Rec. Pow., EW Trans. Pow., SEIS center Z, Magnetic Field Y Selected signals

16. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 16 Veto analysis (4) - Intensity monitor - Example of coincident events Intensity monitor in the power recycling cavity (time series data after data conditioning) Main output Monitor signal

17. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 17 Veto analysis (5) - Seismic motion - Example of coincident events Seismic monitor – center room vertical motion (time series data after data conditioning) Main output Monitor signal

18. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 18 Veto analysis (6) - Magnetic field - Example of coincident events Magnetic field – center room perpend. direction (time series data after data conditioning) Main output Monitor signal

19. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 19 Veto analysis (7) - Veto results - Survival rate Accidental : 4.2% MDAQ 9 signals Accidental : 0.8% HDAQ 3 signals Accidental : 4.4% Total 12 signals Survival rate SNR Threshold Veto results with 178 hours of data

20. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 20 Summary

21. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 21 Summary Systematic survey of monitor signals Data conditioning filter Excess power burst filter Coincidence analysis between main and monitor signals Optimization of analysis parameters Analysis with TAMA DT9 data 200 hours data (10% are used as playground data) Correlations were found in 12 monitor signals (Intensity monitor, Seismic motion, Magnetic field) Reject 92% (SNR>10), 98% (SNR>100) fakes with 4.2% accidental rejection probability Current tasks Hardware signal-injection test  Confirm the safety of veto (already done for some of the monitor signals) Summary

22. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 22 End

23. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 23 Burst-wave analysis (3) - Data conditioning - Data conditioning Line removal AC line, Violin mode peak, Calibration peak Without Line Removal With Line Removal Method FFT 72sec data Reject line freq. components Inverse FFT Normalization Track the drift of noise level  Each spectrum is normalized by averaged noise spectrum Use 30min-averaged spectrum 30min (5.6x10 -4 Hz)

24. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 24 Time series data (after conditioning)

25. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 25 TAMA300 データ解析 (2) - パラメータの選択と解析結果 - パワーフィルタでの解析結果 青 : veto 前 赤 : veto 後 TAMA DT9, Run#140 (200 時間分 ) を解析 時間幅 : 5 通り (1.6msec – 25.6msec) 周波数帯 : 5 通り (500Hz 幅 x3, 1kHz 幅 x2) 以前のパラメータ D t = 12.5 [msec] D f = 2260 [Hz] SNR が最大のものを選び, 閾値と比較

26. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 26 TAMA300 データ解析 (3) - 偽イベント除去 - 強度モニタ信号によるフェイク除去 Off event (accidental) Coincidence 強度モニタ信号も解析, フェイク除去に用いる 時間幅 : 5 通り (1.6msec – 25.6msec) 周波数帯 : 1 通り (200-1500Hz)  重力波チャンネルと同時に閾値以上のものがあれば、イベント候補から除去 F.D: 1% に閾値を設定

27. GWDAW-10 (December 14, 2005, University of Texas at Brownsville, U.S.A.) 27 TAMA300 データ解析 (4) - 偽イベント除去の解析結果 - パワーフィルタでの解析結果 青 : veto 前 赤 : veto 後 TAMA DT9, Run#140 (200 時間分 ) を解析 時間幅 : 5 通り (1.6msec – 25.6msec) 周波数帯 : 5 通り (500Hz 幅 x3, 1kHz 幅 x2) 2 桁程度低減 大きなイベントを 除去できていない