activity
19992016
most citedXMM-Newton observation of the brightest X-ray flare detected so far from SgrA*

216 citations · 800 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.HE2016★ 46 cited

Chandra X-Ray Spectroscopy of the Focused Wind in the Cygnus X-1 System. II. The Nondip Spectrum in the Low/Hard State - Modulations with Orbital Phase

Ivica Miškovičová, Natalie Hell, Manfred Hanke +14

The accretion onto the black hole in the system HDE 226868/Cygnus X-1 is powered by the strong line driven stellar wind of the O-type donor star. We study the X-ray properties of t…

astro-ph.IM2013

In-flight calibration of the INTEGRAL/IBIS mask

S. Soldi, F. Lebrun, A. Gros +9

Since the release of the INTEGRAL Offline Scientific Analysis (OSA) software version 9.0, the ghost busters module has been introduced in the INTEGRAL/IBIS imaging procedure, leadi…

astro-ph.CO2009★ 75 cited

Revealing X-ray obscured quasars in SWIRE sources with extreme mid-IR/optical flux ratios

G. Lanzuisi, E. Piconcelli, F. Fiore +4

Recent works have suggested that selection criteria based on MIR colors can be used to reveal a population of dust-enshrouded, extremely luminous quasars at z>1. However the X-ray…

astro-ph2007★ 29 cited

Linking the X-ray timing and spectral properties of the glitching AXP 1RXS J170849-400910

G. L. Israel, D. Gotz, S. Zane +3

Previous studies of the X-ray flux and spectral properties of 1RXS J170849-400910 showed hints of a possible correlation with the spin glitches that occurred in 1999 and 2001. Howe…

astro-ph2007★ 20 cited

The nature of the infrared counterpart of IGR J19140+0951

D. C. Hannikainen, M. G. Rawlings, P. Muhli +3

The INTEGRAL observatory has been (re-)discovering new X-ray sources since the beginning of nominal operations in early 2003. These sources include X-ray binaries, Active Galactic…

astro-ph2005★ 34 cited

Further evidence for the presence of a neutron star in 4U 2206+54. INTEGRAL and VLA observations

P. Blay, M. Ribo, I. Negueruela +5

The majority of High Mass X-ray Binaries (HMXBs) behave as X-ray pulsars, revealing that they contain a magnetised neutron star. Among the four HMXBs not showing pulsations, and th…