activity
19972019
most citedOn Relativistic Disk Spectroscopy in Compact Objects with X-ray CCD Cameras

68 citations · 147 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2019

Reply to comment on: "An X-ray chimney extending hundreds of parsecs above and below the Galactic Centre"

G. Ponti, F. Hofmann, E. Churazov +5

In response to the comment posted by Nakashima et al. (arXiv:1903.1176), regarding prior claims for the features that we referred to as the Galactic Center Chimneys (2019, Nature,…

astro-ph.HE2011★ 20 cited

Nova M31N 2007-12b: Supersoft X-rays reveal an intermediate polar?

W. Pietsch, M. Henze, F. Haberl +4

For the He/N nova M31N 2007-12b, we analyzed XMM-Newton EPIC and Chandra HRC-I observations of our monitoring program performed at intervals of ten days and added results of a XMM-…

astro-ph.HE2010★ 68 cited

On Relativistic Disk Spectroscopy in Compact Objects with X-ray CCD Cameras

J. M. Miller, A. D'Ai, M. W. Bautz +11

X-ray charge-coupled devices (CCDs) are the workhorse detectors of modern X-ray astronomy. Typically covering the 0.3-10.0 keV energy range, CCDs are able to detect photoelectric a…

astro-ph2003★ 12 cited

RX J004717.4-251811: The first eclipsing X-ray binary outside the Local Group

W. Pietsch, F. Haberl, A. Vogler

The X-ray source RX J004717.4-251811 in the nearby starburst galaxy NGC 253 was found to undergo changes from a low to a high state twice, during an XMM-Newton EPIC observation in…

astro-ph2001★ 46 cited

The X-ray emission of the Intermediate Polar V709 Cas

D. de Martino, G. Matt, K. Mukai +6

We present RXTE and BeppoSAX observations of the Intermediate Polar V709 Cas acquired in 1997 and 1998 respectively. The X-ray emission from 0.1 to 30keV is dominated by the strong…

astro-ph2000

XMM-Newton EPIC Observation of SMC SNR 0102-72.3

M. Sasaki, T. F. X. Stadlbauer, F. Haberl +2

Results from observations of the young oxygen-rich supernova remnant SNR 0102-72.3 in the Small Magellanic Cloud during the calibration phase of the XMM-Newton Observatory are pres…