validation of realistically simulated non-stationary data. soma mukherjee

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Validation of realistically simulated non-stationary data. Soma Mukherjee Centre for Gravitational Wave Astronomy University of Texas at Brownsville. GWDAW9, Annecy, France, 17/12/04 1

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Validation of realistically simulated non-stationary data. Soma Mukherjee Centre for Gravitational Wave Astronomy University of Texas at Brownsville. GWDAW9, Annecy, France, 17/12/04 1. Why model the data ?. - PowerPoint PPT Presentation

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Page 1: Validation of realistically simulated  non-stationary data. Soma Mukherjee

Validation of realistically simulated non-stationary data.

Soma MukherjeeCentre for Gravitational Wave Astronomy

University of Texas at Brownsville.

GWDAW9, Annecy, France, 17/12/04

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Page 2: Validation of realistically simulated  non-stationary data. Soma Mukherjee

Why model the data ? An effort to simulate segments of detector noise such that it has the same

statistical characteristics as the data itself, e.g., it shows same kind of non-stationarity as present in the data.

Non–stationarity can be of different types at different times. We can characterize it near any instant and construct a long stretch of simulated data. Different times will lead to different noise models.

Astrophysical searches estimate efficiency and tune parameters of search algorithms from playground data. Data is non-stationary. E.g. a 60 s stretch of data may not have same value of variance as another 60 s at a later time. Thus any comparison or any estimation work carried out with discretely sampled real data will have bias introduced in it. What we obtain in that case is an ‘average’ value, not instantaneous value.

Certain search algorithms require comparison of different data segments. These are different quantities when data is non-stationary.

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Page 3: Validation of realistically simulated  non-stationary data. Soma Mukherjee

Model outline

Each data segment is divided into three independent components viz. lines, transients and noise floor.

Each component is characterized by low order ARMA model in time domain.

Modeled noise generated from the three independent components are added back together to construct the final product.

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Page 4: Validation of realistically simulated  non-stationary data. Soma Mukherjee

Algorithm : Data

Bandpass

FIR filter

Whiten

Clean Line estimates

Noisefloor

Lines

Second momentEstimation by

Running medianARMA

Model fitData

generation

Demodulate

AmplitudeAnd phase

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Validation : Using KSCD algorithm

KSCD (Kolmogorov-Smirnov Change Point Detector) is a Nonparametric Burst Search algorithm.

Both real data and modeled data is passed through the KSCDpipeline to make comparison.

Rate (triggers per second) vs. Threshold is compared.

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Future :

Application in the triggered and untriggered burst searches.

Library of models for an entire science run.

Incoporate non-linearities: current modeling only valid for secondmoments