activity
20142020
most citedThe role of the reflection fraction in constraining black hole spin

359 citations · 676 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2020★ 6 cited

Modelling X-ray RMS spectra II: the ultra-fast outflow of PDS 456

L. Härer, M. L. Parker, A. Joyce +6

We present an improved model for excess variance spectra describing ultra-fast outflows and successfully apply it to the luminous (L ~ 10^47 erg/s) low-redshift (z = 0.184) quasar…

astro-ph.HE2017★ 30 cited

X-ray reflection from the inner disk of the AGN Ton S180

M. L. Parker, J. M. Miller, A. C. Fabian

We analyse a long archival XMM-Newton observation of the narrow-line Seyfert 1 galaxy Ton S180, using the latest reflection models to explore the high quality X-ray spectrum. We fi…

astro-ph.HE2017★ 8 cited

X-ray Lags in PDS 456 Revealed by Suzaku Observations

Chia-Ying Chiang, E. M. Cackett, A. Zoghbi +5

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 li…

astro-ph.HE2016★ 127 cited

The Soft State of Cygnus X-1 Observed with NuSTAR: A Variable Corona and a Stable Inner Disk

D. J. Walton, J. A. Tomsick, K. K. Madsen +17

We present a multi-epoch hard X-ray analysis of Cygnus X-1 in its soft state based on four observations with NuSTAR. Despite the basic similarity of the observed spectra, there is…

astro-ph.HE2015★ 5 cited

Awakening of The High Redshift Blazar CGRaBS J0809+5341

Vaidehi S. Paliya, M. L. Parker, C. S. Stalin +6

CGRaBS J0809+5341, a high redshift blazar at z = 2.144, underwent a giant optical outburst on 2014 April 19 when it brightened by 5 mag and reached an unfiltered apparent mag…

astro-ph.HE2014★ 26 cited

The changing X-ray time lag in MCG-6-30-15

E. Kara, A. C. Fabian, A. Marinucci +6

MCG-6-30-15 is one of the most observed Narrow Line Seyfert 1 galaxies in the X-ray band. In this paper we examine the X-ray time lags in this source using a total of 600 ks in obs…

astro-ph.HE2014★ 359 cited

The role of the reflection fraction in constraining black hole spin

T. Dauser, J. Garcia, M. L. Parker +2

In many active galaxies, the X-ray reflection features from the innermost regions of the accretion disc are relativistically distorted. This distortion allows us to measure paramet…

astro-ph.HE2014★ 2 cited

Relativistic Disc lines

A. C. Fabian, E. Kara, M. L. Parker

Broad emission lines, particularly broad iron-K lines, are now commonly seen in the X-ray spectra of luminous AGN and Galactic black hole binaries. Sensitive NuSTAR spectra over th…

astro-ph.HE2014★ 113 cited

On the determination of the spin and disc truncation of accreting black holes using X-ray reflection

A. C. Fabian, M. L. Parker, D. R. Wilkins +4

We discuss the application of simple relativistically-blurred X-ray reflection models to the determination of the spin and the inner radius of the disc in accreting black holes. Ob…