activity
20042026
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 13.7k across the 252 of their papers we have counts for

collaborators
Showing astro-phShow all

18 papers · 1 filter

astro-ph2008★ 108 cited

Long term optical and X-ray variability of the Seyfert galaxy Markarian 79

E. Breedt, P. Arévalo, I. M. McHardy +8

We present the results of concurrent X-ray and optical monitoring of the Seyfert 1 galaxy Mrk 79 over a period of more than five years. We find that on short to medium time-scales…

astro-ph2008★ 45 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-ph2008★ 4 cited

A Deep XMM-Newton Observation of the Quasar 3C 287

G. Salvesen, J. M. Miller, E. Cackett +1

We report on an XMM-Newton observation of the z=1.055 quasar and Giga-hertz Peaked Spectrum (GPS) source 3C 287. Our 62.3 ksec observation provides an exceptional X-ray view of a p…

astro-ph2008★ 45 cited

A search for iron emission lines in the Chandra X-ray spectra of neutron star low-mass X-ray binaries

E. M. Cackett, J. M. Miller, J. Homan +6

While iron emission lines are well studied in black hole systems, both in X-ray binaries and Active Galactic Nuclei, there has been less of a focus on these lines in neutron star l…

astro-ph2008★ 6 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-ph2008★ 80 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…