activity
20102026
most citedThe discovery of weak coherent pulsations in the ultraluminous X-ray source NGC 1313 X-2

164 citations · 1.4k across the 33 of their papers we have counts for

collaborators
Showing 2018Show all

7 papers · 1 filter

astro-ph.HE2018★ 1 cited

Relativistic spectroscopy of the extreme NLS1 IRAS13224-3809

M. L. Parker, W. N. Alston, D. J. K Buisson +5

The narrow line Seyfert 1 (NLS1) IRAS 13224-3809 is the most X-ray variable active galactic nucleus (AGN), exhibiting 0.3-10 keV flux changes of over an order of magnitude within a…

astro-ph.HE2018★ 18 cited

AGN feedback in the Phoenix cluster

Ciro Pinto, Christopher J. Bambic, Jeremy S. Sanders +5

Active galactic nuclei (AGN) release a huge amount of energy into the intracluster medium (ICM) with the consequence of offsetting cooling and star formation (AGN feedback) in the…

astro-ph.HE2018★ 23 cited

NuSTAR observations of Mrk 766: distinguishing reflection from absorption

D. J. K. Buisson, M. L. Parker, E. Kara +14

We present two new NuSTAR observations of the narrow line Seyfert 1 (NLS1) galaxy Mrk 766 and give constraints on the two scenarios previously proposed to explain its spectrum and…

astro-ph.HE2018★ 69 cited

Constraints on the Chemical Enrichment History of the Perseus Cluster of Galaxies from High-Resolution X-ray Spectroscopy

A. Simionescu, S. Nakashima, H. Yamaguchi +32

High-resolution spectroscopy of the core of the Perseus Cluster of galaxies, using the satellite above 2 keV and the - Reflection Grating Spectrometer at lowe…

astro-ph.HE2018★ 35 cited

A high-density relativistic reflection origin for the soft and hard X-ray excess emission from Mrk 1044

Labani Mallick, William N. Alston, Michael L. Parker +7

We present the first results from a detailed spectral-timing analysis of a long (130 ks) XMM-Newton observation and quasi-simultaneous NuSTAR and Swift observations of the hi…

astro-ph.HE2018★ 71 cited

The remarkable X-ray variability of IRAS 13224-3809 I: The variability process

W. N. Alston, A. C. Fabian, D. J. K. Buisson +17

We present a detailed X-ray timing analysis of the highly variable NLS1 galaxy, IRAS 13224-3809. The source was recently monitored for 1.5 Ms with XMM-Newton which, combined with 5…