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We investigate how the magnetic loop length of solar flares relates to the timing between their thermal and nonthermal emission signatures. Our study analyzes a sample of 96 C-, M-, and X-class flares observed between 2013 and 2015 with…

太阳与恒星天体物理 · 物理学 2026-02-24 S. M. Perriyil , S. S. Sadangaya , C. G. Giménez de Castro , P. J. A. Simões

X-ray photon correlation spectroscopy (XPCS) is a powerful tool for the investigation of dynamics covering a broad range of time and length scales. The two-time correlation function (TTC) is commonly used to track non-equilibrium dynamical…

软凝聚态物质 · 物理学 2024-06-19 Anastasia Ragulskaya , Vladimir Starostin , Fajun Zhang , Christian Gutt , Frank Schreiber

The gamma-ray sky >100 MeV is dominated by the diffuse emissions from interactions of cosmic rays with the interstellar gas and radiation fields of the Milky Way. Observations of these diffuse emissions provide a tool to study cosmic-ray…

高能天体物理现象 · 物理学 2015-06-04 LAT Collaboration

We present a detailed multi-frequency analysis of an intense monitoring programme of Seyfert 1 galaxy NGC 4593 over a duration of nearly for a month with Swift observatory. We used 185 pointings to study the variability in six…

高能天体物理现象 · 物理学 2019-08-17 Main Pal , Sachindra Naik

The time delay between flux variations in different wavelength bands can be used to probe the inner regions of active galactic nuclei (AGN). Here, we present the first measurements of the time delay between optical and near-infrared (NIR)…

A new method to measure nonlinear dependence between two variables is described using mutual information to analyze the separate linear and nonlinear components of dependence. This technique, which gives an exact value for the proportion of…

信息论 · 计算机科学 2015-12-17 Reginald D. Smith

Disk continuum reverberation mapping is one of the primary ways we learn about active galactic nuclei (AGN) accretion disks. Reverberation mapping assumes that time-varying X-rays incident on the accretion disk drive variability in…

高能天体物理现象 · 物理学 2025-01-14 Amy Secunda , Yan-Fei Jiang , Jenny E. Greene

We investigate the energy-time lag dependence of the source NGC 4593 using XMM-{\it Newton}/EPIC-pn data. We found that the time lag dependency is linear in nature with respect to the logarithm of different energy bands. We also investigate…

高能天体物理现象 · 物理学 2009-07-22 K. Sriram , V. K. Agrawal , A. R. Rao

We have measured the wavelength-dependent lags between the X-ray, UV and optical bands in the high accretion rate ($L/L_{\rm Edd}\approx40\%$) Active Galactic Nucleus Mrk 110 during two intensive monitoring campaigns in February and…

高能天体物理现象 · 物理学 2022-02-09 F. M. Vincentelli , I. McHardy , V. Hernández Santisteban , E. M. Cackett , J. Gelbord , Keith Horne , J. A. Miller , A. Lobban

The inter-band lags among the optical broad-band continua of active galactic nuclei (AGNs) have been intensively explored over the past decade. However, the nature of the lags remains under debate. Here utilizing two distinct scenarios for…

We develop models for time lag between maxima of the source brightness in different wavelengths during a transient flash of luminosity connected with a short period of increase of the mass flux onto the central compact object. We derive a…

太阳与恒星天体物理 · 物理学 2017-03-01 G. S. Bisnovatyi-Kogan , F. Giovannelli

We model the correlated X-ray - UV observations of NGC 7469, for which well sampled data in both these bands have been obtained recently in a multiwavelength monitoring campaign. To this end we derive the transfer function in wavelength \ls…

天体物理学 · 物理学 2009-10-31 Andrew J. Berkley , Demosthenes Kazanas , Jonathan Ozik

Multitime correlation functions provide useful probes for the ensembles of trajectories underlying the stochastic dynamics of complex systems. These can be obtained by measuring their optical response to sequences of ultrashort optical…

软凝聚态物质 · 物理学 2009-11-13 Frantisek Sanda , Shaul Mukamel

We present the analysis of the X-ray variability and spectral timing properties of the ultraluminous X-ray source (ULX) NGC 5408 X-1, one of the most variable ULXs known so far. The variability properties are used as a diagnostic of the…

高能天体物理现象 · 物理学 2015-06-17 B. De Marco , G. Ponti , G. Miniutti , T. Belloni , M. Cappi , M. Dadina , T. Muñoz-Darias

Lags measured from correlated X-ray/UV/optical monitoring of AGN allow us to determine whether UV/optical variability is driven by reprocessing of X-rays or X-ray variability is driven by UV/optical seed photon variations. We present the…

高能天体物理现象 · 物理学 2015-06-22 I. M. McHardy , D. T. Cameron , T. Dwelly , S. Connolly , P. Lira , D. Emmanoulopoulos , J. Gelbord , E. Breedt , P. Arevalo , P. Uttley

To study the neurophysiological basis of attention deficit hyperactivity disorder (ADHD), clinicians use electroencephalography (EEG) which record neuronal electrical activity on the cortex. Instead of focusing on single-channel spectral…

应用统计 · 统计学 2025-06-16 Paolo Victor Redondo , Raphael Huser , Hernando Ombao

Context. Continuum time delays from accretion disks in active galactic nuclei (AGN) has been proposed long time ago as a tool for measuring distances to the monitored sources. However, the method faces serious problems as a number of…

星系天体物理 · 物理学 2023-03-01 Vikram Kumar Jaiswal , Raj Prince , Swayamtrupta Panda , Bożena Czerny

We conduct a molecular dynamics simulation of an inelastic gas system utilizing an event-driven algorithm combined with a thermostat mechanism. Initially, the kinetic energy of the system experiences a decay before settling into a…

计算物理 · 物理学 2025-02-03 Rameez Farooq Shah , Shikha Kumari , Syed Rashid Ahmad

In this paper, we aim to improve multivariate anomaly detection (AD) by modeling the \textit{time-varying non-linear spatio-temporal correlations} found in multivariate time series data . In multivariate time series data, an anomaly may be…

机器学习 · 计算机科学 2025-09-19 Padmaksha Roy , Almuatazbellah Boker , Lamine Mili

In recent years, continuum reverberation mapping involving high cadence UV/optical monitoring campaigns of nearby Active Galactic Nuclei has been used to infer the size of their accretion disks. One of the main results from these campaigns…

星系天体物理 · 物理学 2022-02-02 Edward M. Cackett , Abderahmen Zoghbi , Otho Ulrich