activity
20172020
most citedA deep X-ray view of the bare AGN Ark120. IV. XMM-Newton and NuSTAR spectra dominated by two temperature (warm, hot) Comptonization processes

99 citations · 400 across the 11 of their papers we have counts for

collaborators

12 papers

astro-ph.HE202014 cited

Detection of a possible multiphase ultra-fast outflow in IRAS 13349+2438 with NuSTAR and XMM-Newton

M. L. Parker, G. A. Matzeu, W. N. Alston +6

We present joint NuSTAR and XMM-Newton observations of the bright, variable quasar IRAS 13349+2438. This combined dataset shows two clear iron absorption lines at 8 and 9 keV, whic…

astro-ph.HE202029 cited

The first broadband X-ray view of the narrow line Seyfert 1 Ton S180

G. A. Matzeu, E. Nardini, M. L. Parker +15

We present joint \textit{XMM-Newton} and \textit{NuSTAR} observations of the `bare' narrow line Seyfert 1 Ton S180 (), carried out in 2016 and providing the first hard X-r…

astro-ph.HE202012 cited

X-ray variability analysis of a large series of XMM-Newton + NuSTAR observations of NGC 3227

A. P. Lobban, T. J. Turner, J. N. Reeves +2

We present a series of X-ray variability results from a long XMM-Newton + NuSTAR campaign on the bright, variable AGN NGC 3227. We present an analysis of the lightcurves, showing t…

astro-ph.HE2020

X-ray, UV and optical time delays in the bright Seyfert galaxy Ark 120 with co-ordinated Swift and ground-based observations

A. P. Lobban, S. Zola, U. Pajdosz-Smierciak +17

We report on the results of a multiwavelength monitoring campaign of the bright, nearby Seyfert galaxy, Ark 120 using a ~50-day observing programme with Swift and a ~4-month co-ord…

astro-ph.HE202060 cited

Searching for Ultra-fast Outflows in AGN using Variability Spectra

Z. Igo, M. L. Parker, G. A. Matzeu +8

We present a qualitative search for ultra-fast outflows (UFOs) in excess variance spectra of radio-quiet active galactic nuclei (AGN). We analyse 42 sources from the Tombesi et al.…

astro-ph.HE201942 cited

A deep X-ray view of the bare AGN Ark120. V. Spin determination from disc-Comptonisation efficiency method

D. Porquet, C. Done, J. N. Reeves +13

[Abridged] In our previous work on Ark 120, we found that its 2014 X-ray spectrum is dominated by Comptonisation, while the relativistic reflection emission only originates at tens…