activity
20092019
most citedThe XMM-Newton serendipitous survey. VII. The third XMM-Newton serendipitous source catalogue

354 citations · 1.6k across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.HE2019★ 19 cited

Combining timing characteristics with physical broadband spectral modelling of black hole X-ray binary GX~3394

Riley M. T. Connors, David van Eijnatten, Sera Markoff +6

GX~3394 is a black hole X-ray binary that is a key focus of accretion studies since it goes into outburst roughly every two-to-three years. Tracking of its radio, IR and X-ray f…

astro-ph.IM2018

Feasibility and performance assessment of a practical autonomous deep space navigation system based on X-ray pulsar timing

Setnam Shemar, George Fraser, Lucy Heil +5

Shemar et al. (2016) presented results based on the output of a feasibility study for the European Space Agency (ESA) on the use of X-ray pulsars for deep space navigation, a conce…

astro-ph.IM2017★ 14 cited

Paving the way to simultaneous multi-wavelength astronomy

M. J. Middleton, P. Casella, P. Gandhi +49

Whilst astronomy as a science is historically founded on observations at optical wavelengths, studying the Universe in other bands has yielded remarkable discoveries, from pulsars…

astro-ph.HE2016★ 29 cited

Exploring the Long-Term Evolution of GRS 1915+105

D. Huppenkothen, L. M. Heil, D. W. Hogg +1

Among the population of known galactic black hole X-ray binaries, GRS 1915+105 stands out in multiple ways. It has been in continuous outburst since 1992, and has shown a wide rang…

astro-ph.HE2016★ 195 cited

A quasi-periodic modulation of the iron line centroid energy in the black hole binary H 1743-322

Adam Ingram, Michiel van der Klis, Matthew Middleton +5

Accreting stellar-mass black holes often show a `Type-C' quasi-periodic oscillation (QPO) in their X-ray flux, and an iron emission line in their X-ray spectrum. The iron line is g…

astro-ph.HE2016★ 35 cited

A variable ULX and possible IMBH candidate in M51a

Hannah M. Earnshaw, Timothy P. Roberts, Lucy M. Heil +7

ULX-7, in the northern spiral arm of M51, demonstrates unusual behaviour for an ultraluminous X-ray source, with a hard X-ray spectrum but very high short-term variability. This su…