activity
20072022
most citedPulse phase resolved analysis of the HMXB Cen X-3 over two binary orbits

93 citations · 970 across the 27 of their papers we have counts for

collaborators

31 papers

astro-ph.HE2022★ 11 cited

Common patterns in pulse profiles of High Mass X-ray Binaries

Jaime Alonso-Hernandez, Felix Fuerst, Peter Kretschmar +2

The pulsations of X-ray pulsars carry information about the accretion and magnetic field geometry. Here we present a study and classification of energy resolved pulse profiles of a…

astro-ph.IM2021

INTEGRAL reloaded: spacecraft, instruments and ground system

Erik Kuulkers, Carlo Ferrigno, Peter Kretschmar +85

ESA's INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) was launched on 17 Oct 2002 at 06:41 CEST. Since then, it has been providing long, uninterrupted observations (up t…

astro-ph.HE2020★ 81 cited

Advances in Understanding High-Mass X-ray Binaries with INTEGRAL and Future Directions

Peter Kretschmar, Felix Fürst, Lara Sidoli +48

High mass X-ray binaries are among the brightest X-ray sources in the Milky Way, as well as in nearby Galaxies. Thanks to their highly variable emissions and complex phenomenology,…

astro-ph.HE2017★ 25 cited

Looking at A 0535+26 at low luminosities with NuSTAR

Ralf Ballhausen, Katja Pottschmidt, Felix Fürst +12

We report on two NuSTAR observations of the HMXB A 0535+26 taken toward the end of its normal 2015 outburst at very low keV luminosities of erg/s an…

astro-ph.HE2015★ 21 cited

The Transient Accereting X-Ray Pulsar XTE J1946+274: Stability of the X-Ray Properties at Low Flux and Updated Orbital Solution

Diana M. Marcu-Cheatham, Katja Pottschmidt, Matthias Kühnel +19

We present a timing and spectral analysis of the X-ray pulsar XTE J1946+274 observed with Suzaku during an outburst decline in 2010 October and compare with previous results. XTE J…

astro-ph.HE2013★ 38 cited

XMM-Newton observations of 1A 0535+262 in quiescence

Victor Doroshenko, Andrea Santangelo, Rozaliya Doroshenko +3

Accretion onto magnetized neutron stars is expected to be centrifugally inhibited at low accretion rates. Several sources, however, are known to pulsate in quiescence at luminositi…