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Related papers: Measuring Light Echos in NGC 4051

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NGC 4151 is the brightest Seyfert 1 nucleus in X-rays. It was the first object to show short time delays in the Fe K band, which were attributed to relativistic reverberation, providing a new tool for probing regions at the black hole…

High Energy Astrophysical Phenomena · Physics 2019-10-16 Abderahmen Zoghbi , Jon Miller , Ed Cackett

We present a two-year optical reverberation mapping campaign of NGC 4051, an active galactic nucleus (AGN) hosting a low-mass black hole ($8\times10^5 M_\odot$), using daily observations in seven photometric bands from Las Cumbres…

The wide-band X-ray spectra of the high mass X-ray binary Cygnus X-3 exhibits a pivoting behavior in the `low' (as well as `hard') state, correlated to the radio emission. The time scale of the soft and hard X-rays' anti-correlation, which…

Astrophysics · Physics 2007-05-23 Manojendu Choudhury , A. R. Rao

In previous work, we discussed the detection of reverberation delays in the NLS1 1H0707-495. The delays originate close to the black hole. Here, we show that RE J1034+396 shows very similar lag properties. At low frequencies (< 1 \times…

High Energy Astrophysical Phenomena · Physics 2015-05-30 Abderahmen Zoghbi , Andy Fabian

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

We study the origin of the soft X-ray excess seen in the 'simple' Narrow Line Seyfert 1 galaxy PG1244+026 using all available spectral-timing information. This object shows the standard switch between soft leading the hard band on long…

High Energy Astrophysical Phenomena · Physics 2015-06-19 Emma Gardner , Chris Done

We present ground-based optical photometric monitoring data for NGC 5548, part of an extended multi-wavelength reverberation mapping campaign. The light curves have nearly daily cadence from 2014 January to July in nine filters (\emph{BVRI}…

Over the last years, a number of broadband reverberation mapping campaigns have been conducted to explore the short-term UV and optical variability of nearby AGN. Despite the extensive data collected, the origin of the observed variability…

X-ray reverberation lags from the vicinity of supermassive black holes have been detected in almost 30 AGN. The soft lag, which is the time delay between the hard and soft X-ray light curves, is usually interpreted as the time difference…

High Energy Astrophysical Phenomena · Physics 2017-09-20 Chia-Ying Chiang , E. M. Cackett , A. Zoghbi , A. C. Fabian , E. Kara , M. L. Parker , C. S. Reynolds , D. J. Walton

The variability of the X-ray emission from active galactic nuclei is often characterized using time lags observed between soft and hard energy bands in the detector. The time lags are usually computed using the complex cross spectrum, which…

High Energy Astrophysical Phenomena · Physics 2022-12-07 David C. Baughman , Peter A. Becker

The Seyfert 1 galaxy NGC 4593 was monitored spectroscopically with the Hubble Space Telescope as part of a reverberation mapping campaign that also included Swift, Kepler and ground-based photometric monitoring. During 2016 July 12 - August…

High Energy Astrophysical Phenomena · Physics 2018-04-25 Edward M. Cackett , Chia-Ying Chiang , Ian McHardy , Rick Edelson , Michael R. Goad , Keith Horne , Kirk T. Korista

We present the results from a systematic analysis of the X-ray continuum (`hard') time-lags and intrinsic coherence between the $2-4\,\mathrm{keV}$ and various energy bands in the $0.3-10\,\mathrm{keV}$ range, for ten X-ray bright and…

High Energy Astrophysical Phenomena · Physics 2017-03-14 A. Epitropakis , I. E. Papadakis

We present simultaneous X-ray and optical B and V band light curves of the Seyfert Galaxy NGC3783 spanning 2 years. The flux in all bands is highly variable and the fluctuations are significantly correlated. As shown before by Stirpe et al.…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 P. Arevalo , P. Uttley , P. Lira , E. Breedt , I. M. McHardy , E. Churazov

We exhibit, by compiling all data sets we can acquire, that the Fourier frequency dependent hard X-ray lags, first observed in the analysis of aperiodic variability of the light curves of the black hole candidate Cygnus X-1, appear to be a…

Astrophysics · Physics 2009-10-31 Xin-Min Hua , Demosthenes Kazanas , Wei Cui

On 9-11 May 1998, the highly-variable, low luminosity Seyfert 1 galaxy NGC4051 was observed in an unusual low flux state by BeppoSAX (Guainazzi et al. 1998) RXTE and EUVE. We present fits of the 4-15 keV RXTE spectrum and BeppoSAX MECS…

Astrophysics · Physics 2009-10-31 P. Uttley , I. M. McHardy , I. E. Papadakis , M. Guainazzi , A. Fruscione

We report results from a Suzaku observation of the narrow-line Seyfert 1 NGC 4051. During our observation, large amplitude rapid variability is seen and the averaged 2--10 keV flux is 8.1x10^-12 erg s^-1 cm^-2, which is several times lower…

Reverberation lags in AGN were first discovered in the NLS1 galaxy, 1H0707-495. We present a follow-up analysis using 1.3 Ms of data, which allows for the closest ever look at the reverberation signature of this remarkable source. We…

High Energy Astrophysical Phenomena · Physics 2015-06-11 E. Kara , A. C. Fabian , E. M. Cackett , J. F. Steiner , P. Uttley , D. R. Wilkins , A. Zoghbi

The recent detection of X-ray reverberation lags, especially in the Fe K\alpha\ line region, around Active Galactic Nuclei (AGN) has opened up the possibility of studying the time-resolved response (reflection) of hard X-rays from the…

High Energy Astrophysical Phenomena · Physics 2015-06-17 E. M. Cackett , A. Zoghbi , C. Reynolds , A. C. Fabian , E. Kara , P. Uttley , D. R. Wilkins

We report on a three-year program of coordinated X-ray and optical monitoring of the Narrow-Line Seyfert 1 galaxy NGC 4051. The rapid continuum variations observed in the X-ray spectra are not detected in the optical, although the X-ray and…

Astrophysics · Physics 2009-10-31 B. M. Peterson , I. M. McHardy , B. J. Wilkes

We present the results of X-ray spectral-timing analysis of a 90ks XMM-Newton observation of the nearby, broad line, early-type AGN NGC5273. The X-ray spectrum revealed the clear presence of a reflection component at high energies, with a…

High Energy Astrophysical Phenomena · Physics 2020-01-08 F. M. Vincentelli , G. Mastroserio , I. Mc Hardy , A. Ingram , M. Pahari