activity
20152017
most citedThe response of relativistic outflowing gas to the inner accretion disk of a black hole

146 citations · 315 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2017146 cited

The response of relativistic outflowing gas to the inner accretion disk of a black hole

Michael L. Parker, Ciro Pinto, Andrew C. Fabian +21

Active galactic nucleus (AGN) feedback is the process by which supermassive black holes in the centres of galaxies may moderate the growth of their hosts. Gas outflows from superma…

astro-ph.HE2017124 cited

Properties of AGN coronae in the NuSTAR era II: hybrid plasma

A. C. Fabian, A. Lohfink, R. Belmont +2

The corona, a hot cloud of electrons close to the centre of the accretion disc, produces the hard X-ray power-law continuum commonly seen in luminous Active Galactic Nuclei (AGN).…

astro-ph.HE2016

Relativistic reverberation in the accretion flow of a tidal disruption event

Erin Kara, Jon M. Miller, Chris Reynolds +1

Our current understanding of the curved space-time around supermassive black holes is based on actively accreting black holes, which make up only ten per cent or less of the overal…

astro-ph.GA2016

The rhythm of Fairall 9 -- I: Observing the spectral variability with XMM-Newton and NuSTAR

Anne Lohfink, Christopher Reynolds, Ciro Pinto +13

We present a multi-epoch X-ray spectral analysis of the Seyfert 1 galaxy Fairall 9. Our analysis shows that Fairall 9 displays unique spectral variability in that its ratio residua…

astro-ph.HE20158 cited

Properties of AGN coronae in the NuSTAR era

A. C. Fabian, A. Lohfink, E. Kara +3

The focussing optics of NuSTAR have enabled high signal-to-noise spectra to be obtained from many X-ray bright Active Galactic Nuclei (AGN) and Galactic Black Hole Binaries (BHB).…

astro-ph.HE201537 cited

The Compton hump and variable blue wing in the extreme low-flux NuSTAR observations of 1H0707-495

E. Kara, A. C. Fabian, A. M. Lohfink +10

The Narrow-line Seyfert I galaxy, 1H0707-495, has been well observed in the 0.3-10 keV band, revealing a dramatic drop in flux in the iron K alpha band, a strong soft excess, and s…