activity
20102026
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 9.7k across the 184 of their papers we have counts for

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Showing 2013Show all

8 papers · 1 filter

astro-ph.HE2013★ 139 cited

Modelling the broad Fe Kα reverberation in the AGN NGC 4151

E. M. Cackett, A. Zoghbi, C. Reynolds +4

The recent detection of X-ray reverberation lags, especially in the Fe Kα line region, around Active Galactic Nuclei (AGN) has opened up the possibility of studying the time-resolv…

astro-ph.HE2013★ 54 cited

The curious time lags of PG 1244+026: Discovery of the iron K reverberation lag

E. Kara, E. M. Cackett, A. C. Fabian +2

High-frequency iron K reverberation lags, where the red wing of the line responds before the line centroid, are a robust signature of relativistic reflection off the inner accretio…

astro-ph.HE2013★ 33 cited

Principal Component Analysis of MCG--6-30-15 with XMM-Newton

M. L. Parker, A. Marinucci, L. Brenneman +4

We analyse the spectral variability of MCG--06-30-15 with 600 ks of XMM-Newton data, including 300 ks of new data from the joint XMM-Newton and NuSTAR 2013 observational campaign.…

astro-ph.HE2013★ 37 cited

Hard X-ray Lags in Active Galactic Nuclei: Testing the Distant Reverberation Hypothesis with NGC 6814

D. J. Walton, A. Zoghbi, E. M. Cackett +7

We present an X-ray spectral and temporal analysis of the variable active galaxy NGC 6814, observed with Suzaku during November 2011. Remarkably, the X-ray spectrum shows no eviden…

astro-ph.HE2013★ 132 cited

Discovery of high-frequency iron K lags in Ark 564 and Mrk 335

E. Kara, A. C. Fabian, E. M. Cackett +3

We use archival XMM-Newton observations of Ark 564 and Mrk 335 to calculate the frequency dependent time-lags for these two well-studied sources. We discover high-frequency Fe K la…

astro-ph.HE2013★ 15 cited

The Hot and Energetic Universe: The close environments of supermassive black holes

Michal Dovciak, Giorgio Matt, Stefano Bianchi +22

Most of the action in Active Galactic Nuclei (AGN) occurs within a few tens of gravitational radii from the supermassive black hole, where matter in the accretion disk may lose up…