We report the discovery of hard X-ray delays in the X-ray emission of the Seyfert 1 galaxy Mrk 110, based on a long XMM-Newton observation. Cross-correlation between the X-ray light curves of different energy bands reveals an energy-dependent delay ranging from a few minutes to an hour. We find that the energy spectrum can be modeled by Comptonization of disk blackbody photons. The energy-dependent delay can be modeled as due to the effect of Comptonization in a hot plasma confined within 10 Schwarzschild radii of the black hole. We discuss our results in the context of inverse Comptonization of the soft photons by highly energetic plasma
We use the XMM–Newton EPIC-pn instrument in timing mode to extend spectral time-lag studies of hard ...
International audienceAims:We propose a reflection model of the time delays detected during an excep...
We present an XMM-Newton time-resolved spectral analysis of the narrow-line Seyfert 1 galaxy Mrk 766...
The broadband X-ray emission from type 1 active galactic nuclei, dominated by a power-law continuum,...
The origin of the observed time lags, in nearby active galactic nuclei (AGNs), between hard and soft...
4 pages, 3 figuresWe present a Comptonization model for the observed properties of the energy-depend...
Using a Monte Carlo method, we derive spectra arising from Comptonization taking place close to a Ke...
International audienceWe demonstrate that an X-ray spectrum of a converging inflow (CI) onto a black...
We have analyzed the timing properties of the Narrow-line Seyfert 1 galaxy Mrk 766 observed with XMM...
Reverberation from scattering material around the black hole in active galactic nuclei is expected t...
Using new XMM–Newton observations we detect hard X-ray time lags in the rapid variability of the Com...
We present the first results from a detailed spectral-timing analysis of a long (~130 ks) XMM- Newto...
We used a ~300 ks long XMM-Newton observation of the Seyfert 1 galaxy MCG-6-30-15 to study the corre...
We study the energy dependent photon variability from a thermal Comptonizing plasma that is oscillat...
Results of Monte Carlo simulations of the Comptonization of photons in a finite spherical Comptonizi...
We use the XMM–Newton EPIC-pn instrument in timing mode to extend spectral time-lag studies of hard ...
International audienceAims:We propose a reflection model of the time delays detected during an excep...
We present an XMM-Newton time-resolved spectral analysis of the narrow-line Seyfert 1 galaxy Mrk 766...
The broadband X-ray emission from type 1 active galactic nuclei, dominated by a power-law continuum,...
The origin of the observed time lags, in nearby active galactic nuclei (AGNs), between hard and soft...
4 pages, 3 figuresWe present a Comptonization model for the observed properties of the energy-depend...
Using a Monte Carlo method, we derive spectra arising from Comptonization taking place close to a Ke...
International audienceWe demonstrate that an X-ray spectrum of a converging inflow (CI) onto a black...
We have analyzed the timing properties of the Narrow-line Seyfert 1 galaxy Mrk 766 observed with XMM...
Reverberation from scattering material around the black hole in active galactic nuclei is expected t...
Using new XMM–Newton observations we detect hard X-ray time lags in the rapid variability of the Com...
We present the first results from a detailed spectral-timing analysis of a long (~130 ks) XMM- Newto...
We used a ~300 ks long XMM-Newton observation of the Seyfert 1 galaxy MCG-6-30-15 to study the corre...
We study the energy dependent photon variability from a thermal Comptonizing plasma that is oscillat...
Results of Monte Carlo simulations of the Comptonization of photons in a finite spherical Comptonizi...
We use the XMM–Newton EPIC-pn instrument in timing mode to extend spectral time-lag studies of hard ...
International audienceAims:We propose a reflection model of the time delays detected during an excep...
We present an XMM-Newton time-resolved spectral analysis of the narrow-line Seyfert 1 galaxy Mrk 766...