activity
19962015
most citedThe XMM-Newton Serendipitous Survey. V. The Second XMM-Newton Serendipitous Source Catalogue

489 citations · 3.2k across the 65 of their papers we have counts for

collaborators

66 papers

astro-ph.HE2015★ 139 cited

The population of X-ray supernova remnants in the Large Magellanic Cloud

P. Maggi, F. Haberl, P. J. Kavanagh +11

We present a comprehensive X-ray study of the population of supernova remnants (SNRs) in the LMC. Using primarily XMM-Newton, we conduct a systematic spectral analysis of LMC SNRs…

astro-ph.SR2014★ 39 cited

Recurrent Novae in M31

A. W. Shafter, M. Henze, T. A. Rector +8

The reported positions of 964 suspected nova eruptions in M31 recorded through the end of calendar year 2013 have been compared in order to identify recurrent nova candidates. To p…

astro-ph.HE2013★ 75 cited

X-ray monitoring of classical novae in the central region of M31. III. Autumn and winter 2009/10, 2010/11 and 2011/12

M. Henze, W. Pietsch, F. Haberl +7

[Abridged] Classical novae (CNe) represent the major class of supersoft X-ray sources (SSSs) in the central region of our neighbouring galaxy M31. We performed a dedicated monitori…

astro-ph.HE2013★ 34 cited

Four new X-ray-selected supernova remnants in the Large Magellanic Cloud

P. Maggi, F. Haberl, P. J. Kavanagh +8

Aims: We present a detailed multi-wavelength study of four new supernova remnants (SNRs) in the Large Magellanic Cloud (LMC). The objects were identified as SNR candidates in X-ray…

astro-ph.HE2013★ 24 cited

Swift J053041.9-665426, a new Be/X-ray binary pulsar in the Large Magellanic Cloud

G. Vasilopoulos, P. Maggi, F. Haberl +4

We observed the newly discovered X-ray source Swift J053041.9-665426 in the X-ray and optical regime to confirm its proposed nature as a high mass X-ray binary. We obtained XMM-New…

astro-ph.HE2013★ 11 cited

AGN behind the SMC selected from radio and X-ray surveys

R. Sturm, D. Drašković, M. D. Filipović +8

The XMM-Newton survey of the Small Magellanic Cloud (SMC) revealed 3053 X-ray sources with the majority expected to be active galactic nuclei (AGN) behind the SMC. However, the hig…