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Open AccessJournal ArticleDOI

A heuristic derivation of the uncertainty for frequency determination in time series data

Thomas Kallinger, +2 more
- 01 Apr 2008 - 
- Vol. 481, Iss: 2, pp 571-574
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TLDR
In this paper, a simple, but realistic, estimate of the frequency uncertainty in time-series analyses is presented, which is based on a simple formula for the upper limit of the amplitude, frequency, and phase uncertainties.
Abstract
Context. Several approaches to estimating frequency, phase, and amplitude errors in time-series analyse have been reported in the literature, but they are either time-consuming to compute, grossly overestimating the error, or are based on empirically determined criteria.Aims. A simple, but realistic estimate of the frequency uncertainty in time-series analyses is our goal here.Methods. Synthetic data sets with mono- and multi-periodic harmonic signals and with randomly distributed amplitude, frequency, and phase were generated and white noise added. We tried to recover the input parameters with classical Fourier techniques and investigated the error as a function of the relative level of noise, signal, and frequency difference.Results. We present simple formulas for the upper limit of the amplitude, frequency, and phase uncertainties in time-serie analyses. We also demonstrate the possibility of detecting frequencies that are separated by less than the classical frequency resolution and of finding that the realistic frequency error is at least 4 times smaller than the classical frequency resolution.

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TL;DR: BRITE-Constellation as mentioned in this paper is an international nanosatellite mission to monitor photometrically, in two colours, the brightness and temperature variations of stars generally brighter than mag(V) ≈ 4 with precision and time coverage not possible from the ground.
Journal ArticleDOI

BRITE-Constellation: nanosatellites for precision photometry of bright stars

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Asteroseismic analysis of the CoRoT \delta-Scuti star HD174936

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References
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Journal ArticleDOI

Fourier analysis with unequally-spaced data*

TL;DR: In this article, a discrete Fourier transform for arbitrary data spacing is defined, and the pathology of the data spacing, including aliasing and related effects, is shown to be contained in the spectral window.
Journal ArticleDOI

SigSpec. I. Frequency- and phase-resolved significance in Fourier space

TL;DR: SigSpec as mentioned in this paper is based on an analytical solution of the probability that a DFT peak of a given amplitude does not arise from white noise in a non-equally spaced data set.
Journal ArticleDOI

An Upper Limit on the Albedo of HD 209458b: Direct Imaging Photometry with the MOST Satellite

TL;DR: In this article, the authors presented a space-based photometry of the transiting exoplanetary system HD 209458 obtained with the Microvariablity and Oscillations of Stars (MOST) satellite, spanning 14 days and covering 4 transits and 4 secondary eclipses.
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