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Related papers: X-Ray Variability Coherence in the Time Domain

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Quantities characterizing temporal property, e.g. power density, coherence, and time lag, can be defined and calculated directly in the time domain without using the Fourier transformation. Spectral hardness, variability duration, and…

Astrophysics · Physics 2017-11-01 Ti-pei Li

We describe how the coherence function, a Fourier frequency-dependent measure of the linear correlation between time series measured simultaneously in two energy channels, can be used in conjunction with energy spectra, power spectra, and…

Astrophysics · Physics 2009-10-28 Brian A. Vaughan , Michael A. Nowak

The interpretation of Fourier spectra in the time domain is critically examined. Power density spectra defined and calculated in the time domain are compared with Fourier spectra in the frequency domain for three different types of…

Astrophysics · Physics 2009-11-07 T. P. Li , Y. Muraki

A technique for timescale analysis of spectral lags performed directly in the time domain is developed. Simulation studies are made to compare the time domain technique with the Fourier frequency analysis for spectral time lags. The time…

Astrophysics · Physics 2014-10-13 T. P. Li , J. L. Qu , H. Feng , L. M. Song , G. Q. Ding , L. Chen

There have been a number of recent spectral models that have been successful in reproducing the observed X-ray spectra of galactic black hole candidates (GBHC). However, there still exists controversy over such issues as: what are the…

Astrophysics · Physics 2015-06-24 M. A. Nowak , J. B. Dove , B. A. Vaughan , M. C. Begelman

We present the most extensive analysis of Fourier-based X-ray timing properties of the black hole binary Cygnus X-1 to date, based on 12 years of bi-weekly monitoring with RXTE from 1999 to 2011. Our aim is a comprehensive study of timing…

We have developed an algorithm that, starting from the observed properties of the X-ray spectrum and fast variability of an X-ray binary allows the production of synthetic data reproducing observables such as power density spectra and time…

High Energy Astrophysical Phenomena · Physics 2015-05-19 Y. X. Wu , T. M. Belloni , L. Stella

A technique of timescale analysis performed directly in the time domain has been developed recently. We have applied the technique to studying rapid variabilities of hard X-rays from neutron star and black hole binaries, gamma-ray bursts…

Astrophysics · Physics 2016-01-27 T. P. Li

To better constrain the emission mechanism underlying the hard state of galactic black hole candidates, we use high-time resolution RXTE lightcurves for Cyg X-1 and GX 399-4 to compute two higher order variability statistics for these…

Astrophysics · Physics 2009-11-07 Thomas J. Maccarone , Paolo S. Coppi

The X-ray signal from active galactic nuclei and black hole X-ray binaries is highly variable on a range of timescales. This variability can be exploited to map the region of interest close to the black hole, which is far too small to…

High Energy Astrophysical Phenomena · Physics 2023-05-24 Adam Ingram

We present simultaneous multi-band radio and X-ray observations of the black hole X-ray binary Cygnus X-1, taken with the Karl G. Jansky Very Large Array and the Nuclear Spectroscopic Telescope Array. With these data, we detect clear flux…

High Energy Astrophysical Phenomena · Physics 2019-01-23 A. J. Tetarenko , P. Casella , J. C. A. Miller-Jones , G. R. Sivakoff , B. E. Tetarenko , T. J. Maccarone , P. Gandhi , S. Eikenberry

I discuss some practical aspects of the analysis of millisecond time variability X-ray data obtained from accreting neutron stars and black holes. First I give an account of the statistical methods that are at present commonly applied in…

Astrophysics · Physics 2007-05-23 M. van der Klis

We present first results from the spectral and temporal analysis of an RXTE monitoring campaign of the black hole candidate Cygnus X-1 in 1999. The timing properties of this hard state black hole show considerable variability, even though…

Astrophysics · Physics 2009-10-31 K. Pottschmidt , J. Wilms , R. Staubert , M. A. Nowak , J. B. Dove , W. A. Heindl , D. M. Smith

We develop new techniques to deconvolve the radial structure of the X-ray emission region in the bright low/hard state of the black hole Cygnus X-1 using both spectral and timing data in the 3-35~keV range. The spectrum at these energies is…

High Energy Astrophysical Phenomena · Physics 2018-08-31 Ra'ad D. Mahmoud , Chris Done

We investigate the variability of Cygnus X-1 in the context of shot moise models, and employ a peak detection algorithm to select individual shots. For a long observation of the low, hard state, the distribution of time intervals between…

Astrophysics · Physics 2009-11-13 Warren Focke , Jean Swank , Larry Wai

A variety of statistical methods for understanding variability in the time domain for low count rate X-ray and gamma-ray sources are explored. Variability can be detected using nonparametric (Anderson-Darling and overdispersion tests) and…

Instrumentation and Methods for Astrophysics · Physics 2023-05-24 Eric D. Feigelson , Vinay L. Kashyap , Aneta Siemiginowska

In the past decades, the phenomenology of fast time variations of high-energy flux from black-hole binaries has increased, thanks to the availability of more and more sophisticated space observatories, and a complex picture has emerged.…

High Energy Astrophysical Phenomena · Physics 2019-02-19 Tomaso M. Belloni

This paper proposes a frequency domain approach to test the hypothesis that a complex-valued vector time series is proper, i.e., for testing whether the vector time series is uncorrelated with its complex conjugate. If the hypothesis is…

Methodology · Statistics 2017-04-05 Swati Chandna , Andrew T. Walden

Analyzing time series in the frequency domain enables the development of powerful tools for investigating the second-order characteristics of multivariate processes. Parameters like the spectral density matrix and its inverse, the coherence…

Methodology · Statistics 2024-01-19 Jonas Krampe , Efstathios Paparoditis

We present calculations of the time lags and the coherence function of X-ray photons for a novel model of radiation emission from accretion powered, high-energy sources. Our model involves only Comptonization of soft photons injected near…

Astrophysics · Physics 2009-10-30 Xin-Min Hua , Demosthenes Kazanas , Lev Titarchuk
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