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

146 citations · 454 across the 7 of their papers we have counts for

collaborators

9 papers

astro-ph.HE201780 cited

Reflection Spectra of the Black Hole Binary Candidate MAXI J1535-571 in the Hard State Observed by NuSTAR

Yanjun Xu, Fiona A. Harrison, Javier A. Garcia +9

We report on a NuSTAR observation of the recently discovered bright black hole candidate MAXI J1535-571. NuSTAR observed the source on MJD 58003 (five days after the outburst was r…

astro-ph.HE201736 cited

Using principal component analysis to understand the variability of PDS 456

M. L. Parker, J. N. Reeves, G. A. Matzeu +2

We present a spectral-variability analysis of the low-redshift quasar PDS 456 using principal component analysis. In the XMM-Newton data, we find a strong peak in the first princip…

astro-ph.HE201723 cited

Disentangling the Complex Broadband X-ray Spectrum of IRAS 13197-1627 with NuSTAR, XMM-Newton and Suzaku

D. J. Walton, M. Brightman, G. Risaliti +8

We present results from a coordinated -+ observation of the type 1.8 Seyfert galaxy IRAS 13197-1627. This is a highly complex source, with strong contributions…

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

Broadband Observations of High Redshift Blazars

Vaidehi S. Paliya, M. L. Parker, A. C. Fabian +1

We present a multi-wavelength study of four high redshift blazars, S5 0014+81 (), CGRaBS J0225+1846 (), BZQ J1430+4205 (), and 3FGL J1656.23303 (