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

16 papers

astro-ph.HE2009207 cited

The Fundamental Plane of Accretion Onto Black Holes with Dynamical Masses

Kayhan Gultekin, Edward M. Cackett, Jon M. Miller +3

Black hole accretion and jet production are areas of intensive study in astrophysics. Recent work has found a relation between radio luminosity, X-ray luminosity, and black hole ma…

astro-ph.HE20095 cited

The Behavior of Matter under Extreme Conditions

F. Paerels, M. Mendez, M. Agueros +29

The cores of neutron stars harbor the highest matter densities known to occur in nature, up to several times the densities in atomic nuclei. Similarly, magnetic field strengths can…

astro-ph.HE2009137 cited

Broad relativistic iron emission line observed in SAX J1808.4-3658

E. M. Cackett, D. Altamirano, A. Patruno +4

During the September-October 2008 outburst of the accreting millisecond pulsar SAX J1808.4-3658, the source was observed by both Suzaku and XMM-Newton approximately 1 day apart. Sp…

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…