activity
20042009
most citedTesting thermal reprocessing in AGN accretion discs

299 citations · 1.8k across the 14 of their papers we have counts for

collaborators
Showing astro-phShow all

13 papers · 1 filter

astro-ph200845 cited

Chandra and Swift observations of the quasi-persistent neutron star transient EXO 0748-676 back to quiescence

N. Degenaar, R. Wijnands, M. T. Wolff +8

The quasi-persistent neutron star X-ray transient and eclipsing binary EXO 0748-676 recently started the transition to quiescence following an accretion outburst that lasted more t…

astro-ph20086 cited

Science with the XEUS High Time Resolution Spectrometer

D. Barret, T. Belloni, S. Bhattacharyya +12

XEUS has been recently selected by ESA for an assessment study. XEUS is a large mission candidate for the Cosmic Vision program, aiming for a launch date as early as 2018. XEUS is…

astro-ph200880 cited

Cooling of the crust in the neutron star low-mass X-ray binary MXB 1659-29

Edward M. Cackett, Rudy Wijnands, Jon M. Miller +2

In quasi-persistent neutron star transients, long outbursts cause the neutron star crust to be heated out of thermal equilibrium with the rest of the star. During quiescence, the c…

astro-ph200893 cited

Initial Measurements of Black Hole Spin in GX 339-4 from Suzaku Spectroscopy

J. M. Miller, C. S. Reynolds, A. C. Fabian +6

We report on a deep Suzaku observation of the stellar-mass black hole GX 339-4 in outburst. A clear, strong, relativistically-shaped iron emission line from the inner accretion dis…

astro-ph2007170 cited

Relativistic iron emission lines in neutron star low-mass X-ray binaries as probes of neutron star radii

Edward M. Cackett, Jon M. Miller, Sudip Bhattacharyya +6

Using Suzaku observations of three neutron star low-mass X-ray binaries (Ser X-1, 4U 1820-30 and GX 349+2) we have found broad, asymmetric, relativistic Fe K emission lines in all…

astro-ph2007299 cited

Testing thermal reprocessing in AGN accretion discs

E. M. Cackett, K. Horne, H. Winkler

The thermal reprocessing hypothesis in AGN, where EUV/X-ray photons are reprocessed by the accretion disc into optical/UV photons, predicts wavelength-dependent time delays between…