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We present the first intensive continuum reverberation mapping study of the high accretion rate Seyfert galaxy Mrk 110. The source was monitored almost daily for more than 200 days with the Swift X-ray and UV/optical telescopes, supported…

Time-correlated noise is a significant source of uncertainty when modeling exoplanet light-curve data. A correct assessment of correlated noise is fundamental to determine the true statistical significance of our findings. Here we review…

地球与行星天体物理 · 物理学 2016-12-21 Patricio Cubillos , Joseph Harrington , Thomas J. Loredo , Nate B. Lust , Jasmina Blecic , Madison Stemm

Most statistical inference from cosmic large-scale structure relies on two-point statistics, i.e.\ on the galaxy-galaxy correlation function (2PCF) or the power spectrum. These statistics capture the full information encoded in the Fourier…

宇宙学与河外天体物理 · 物理学 2023-06-09 Kamran Ali , Danail Obreschkow , Cullan Howlett , Camille Bonvin , Claudio Llinares , Felipe Oliveira Franco , Chris Power

In this paper, standard accretion disk models of AGNs are tested using light curves of 26 objects well observed for reverberation mapping. Time scales of variations are estimated by the most common definition of the variability time scale…

天体物理学 · 物理学 2014-01-10 H. T. Liu , J. M. Bai , X. H. Zhao , L. Ma

Variability in the X-rays is a key ingredient in understanding and unveiling active galactic nuclei (AGN) properties. In this band flux variations occur on short time scales (hours) as well as on larger times scales. While short time scale…

高能天体物理现象 · 物理学 2017-03-08 R. Middei , F. Vagnetti , S. Bianchi , F. La Franca , M. Paolillo , F. Ursini

In a previous paper, we studied two statistical methods used to analyse the variability of active galactic nuclei (AGNs): the C and F statistics. Applying them to observed differential light-curves of 39 AGNs, we found that, even though the…

星系天体物理 · 物理学 2020-09-02 L. Zibecchi , I. Andruchow , S. A. Cellone , D. D. Carpintero

In multivariate time series systems, lead-lag relationships reveal dependencies between time series when they are shifted in time relative to each other. Uncovering such relationships is valuable in downstream tasks, such as control,…

统计金融 · 定量金融 2023-09-19 Yichi Zhang , Mihai Cucuringu , Alexander Y. Shestopaloff , Stefan Zohren

In this study, we demonstrate some of the caveats in common statistical methods used for analysing astronomical variability timescales. We consider these issues specifically in the context of active galactic nuclei (AGNs) and use a more…

星系天体物理 · 物理学 2024-12-12 Sofia Kankkunen , Merja Tornikoski , Talvikki Hovatta

We have obtained high time resolution (seconds) photometry of LMC X-2 in December 1997, simultaneously with the Rossi X-ray Timing Explorer (RXTE), in order to search for correlated X-ray and optical variability on timescales from seconds…

天体物理学 · 物理学 2009-11-10 Katherine E. McGowan , Phil A. Charles , Darragh O'Donoghue , Alan P. Smale

Continuum reverberation mapping (RM) is a powerful technique for constraining the accretion disk structure in active galactic nuclei (AGNs). In typical cases, the shorter-wavelength emission is used as the reference, and a positive time lag…

星系天体物理 · 物理学 2026-05-05 Chen MuLin , Cheng PeiZhen , Chen XingQian , Gu Ying , Zheng Qi , Liao GuiLin , Zhang XueGuang

Aperiodic variability is a characteristic feature of young stars, massive stars, and active galactic nuclei. With the recent proliferation of time domain surveys, it is increasingly essential to develop methods to quantify and analyze…

天体物理仪器与方法 · 物理学 2026-04-01 Krzysztof Findeisen , Ann Marie Cody , Lynne Hillenbrand

We have used the Fourier cross spectra of Cyg X-1, as obtained with BATSE during a period of almost 2000 days, to estimate the phase (or time) lags between X-ray flux variations in the 20-50 keV and the 50-100 keV bands as a function of…

We are conducting an archival Swift program to measure multiwavelength variability in active galactic nuclei (AGN). This variability information will provide constraints on the geometry, physical conditions and processes of the structures…

高能天体物理现象 · 物理学 2015-05-21 Jonathan Gelbord , Caryl Gronwall , Dirk Grupe , Dan Vanden Berk , Jian Wu

Changing-look active galactic nuclei (CL AGNs) show large changes in luminosity and optical spectral state on time-scales of a few years, and provide a valuable probe of time-dependent accretion in the disc-BLR-torus system. We present a…

星系天体物理 · 物理学 2026-03-19 Yu Tao , Jie Tang , Xuan Wei

The long-time behavior of the velocity autocorrelation function (VACF) is investigated by the molecular dynamics simulation of a two-dimensional system which has both a many-body interaction and a random potential. With strengthening the…

统计力学 · 物理学 2009-11-13 Tatsuro Yuge , Akira Shimizu

MCG-6-30-15 is one of the most observed Narrow Line Seyfert 1 galaxies in the X-ray band. In this paper we examine the X-ray time lags in this source using a total of 600 ks in observations (440 ks exposure) taken with the XMM-Newton…

高能天体物理现象 · 物理学 2015-06-22 E. Kara , A. C. Fabian , A. Marinucci , G. Matt , M. L. Parker , W. Alston , L. W. Brenneman , E. M. Cackett , G. Miniutti

We introduce a two-particle correlation function (2PCF) for the Milky Way, constructed to probe spatial correlations in the orthogonal directions of the stellar disk in the Galactic cylindrical coordinates of $R$, $\phi$, and $z$. We use…

星系天体物理 · 物理学 2023-01-16 Austin Hinkel , Susan Gardner , Brian Yanny

We present reverberation mapping measurements for the prominent ultraviolet broad emission lines of the active galactic nucleus Mrk817 using 165 spectra obtained with the Cosmic Origins Spectrograph on the Hubble Space Telescope. Our…

Variable continuum emission from AGN can be used to probe the structure of their accretion disks via reverberation mapping. Assuming a variable, hot inner light source irradiates the surrounding accretion disk, time delays between different…

Using new XMM-Newton observations we detect hard X-ray time lags in the rapid variability of the Compton-thin Seyfert 2 galaxy IRAS 18325-5926. The higher-energy X-ray variations lag behind correlated lower-energy variations by up to ~3ks…

高能天体物理现象 · 物理学 2015-06-22 Andrew Lobban , William Alston , Simon Vaughan