Many experiments, and in particular gravitational wave detectors, produce continuous streams of data whose frequency representations contain discrete, relatively narrowband coherent features at high amplitude. We discuss the application of digital Fourier transforms (DFTs) to characterization of these features, hereafter frequently referred to as lines. Application of DFTs to continuously produced time-domain data is achieved through an algorithm [7], hereafter referred to as EFC*, for efficient time-domain determination of the Fourier coefficients of a data set. We first define EFC and discuss parameters relating to the algorithm that determine its properties and action on the data. In gravitational wave interferometers, these lines are co...
Some practical extensions to digital signal processing techniques are presented. Firstly, an account...
The space-based gravitational wave detector LISA will observe in the low-frequency gravitational-wav...
Author Institution: Department of Physics and Astronomy, University of WyomingThe discrete Fourier t...
Many experiments, and in particular gravitational wave detectors, produce continuous streams of data...
We describe a new technique for removing troublesome interference from external coherent signals pre...
We describe a procedure to identify and remove a class of non-stationary and non-harmonic interferen...
We describe a procedure to identify and remove a class of nonstationary and nonharmonic interference...
We describe a procedure to identify and remove a class of interference lines from gravitational wave...
The direct detection of continuous gravitational waves from pulsars is a much anticipated discovery ...
We present the Fourier Transform of the data output of gravitational wave laser interferometer for c...
Abstract. We demonstrate the usefulness of some signal-processing tools for the EISCAT data analysis...
This article discusses the potential advantages of a data processing technique for continuous gravit...
Spelling mistake corrected in one author\'s nameNetwork data analysis methods are the only way to pr...
I present a new method to remove detector noise from gravitationalwave (GW) interferometer data in t...
All electrical signals can be described either as a function of time or of frequency. When we observ...
Some practical extensions to digital signal processing techniques are presented. Firstly, an account...
The space-based gravitational wave detector LISA will observe in the low-frequency gravitational-wav...
Author Institution: Department of Physics and Astronomy, University of WyomingThe discrete Fourier t...
Many experiments, and in particular gravitational wave detectors, produce continuous streams of data...
We describe a new technique for removing troublesome interference from external coherent signals pre...
We describe a procedure to identify and remove a class of non-stationary and non-harmonic interferen...
We describe a procedure to identify and remove a class of nonstationary and nonharmonic interference...
We describe a procedure to identify and remove a class of interference lines from gravitational wave...
The direct detection of continuous gravitational waves from pulsars is a much anticipated discovery ...
We present the Fourier Transform of the data output of gravitational wave laser interferometer for c...
Abstract. We demonstrate the usefulness of some signal-processing tools for the EISCAT data analysis...
This article discusses the potential advantages of a data processing technique for continuous gravit...
Spelling mistake corrected in one author\'s nameNetwork data analysis methods are the only way to pr...
I present a new method to remove detector noise from gravitationalwave (GW) interferometer data in t...
All electrical signals can be described either as a function of time or of frequency. When we observ...
Some practical extensions to digital signal processing techniques are presented. Firstly, an account...
The space-based gravitational wave detector LISA will observe in the low-frequency gravitational-wav...
Author Institution: Department of Physics and Astronomy, University of WyomingThe discrete Fourier t...