Add to ORKGThe analysis of the broad iron line profile in the X-ray spectra of active galactic nuclei and black hole X-ray binaries allows us to constrain the spin parameter of the black hole. We compare the constraints on the spin value for two X-ray sources, MCG-6-30-15 and GX 339-4, with a broad iron line using present relativistic line models in XSPEC - LAOR and KYRLINE
Future X-ray instrumentation is expected to allow us to significantly improve the constraints derive...
We show that disc continuum fitting can be used to constrain black hole spin in a subclass of narrow...
Using the 770 ks XMM-Newton survey of the Lockman Hole field in combination with extensive optical i...
We discuss black hole spin measurements employing the relativistic iron line profiles in the X-ray d...
Accretion disk reflection spectra, including broad iron emission lines, bear the imprints of the str...
We present an analysis of the observed broad iron line feature and putative warm absorber in the lon...
4 pages, 3 color figures, subm. to ApJWe report on a deep Suzaku observation of the stellar-mass bla...
We fit X-ray spectral data in the thermal dominant or high soft state of two dynamically confirmed b...
The 6.4\,keV Iron reflection line possesses strong diagnostic potential for AGN-systems. In the rare...
Several AGN and black hole X-ray binaries show a clear very broad iron line which is strong evidence...
The micro Seyfert galaxy NGC-4395 hosts a supermassive black hole at its center that actively accret...
International audienceThe interpretation of very broad iron lines in the X-ray spectra of Active Gal...
This dissertation explores the question of whether broad iron lines from the accretion disk can be u...
Recent X-ray spectroscopy made with ASCA have shown broad, skewed iron line emission from Seyfert-1 ...
The Galactic black hole candidate XTE J1752−223 was observed during the decay of its 2009 outburst w...
Future X-ray instrumentation is expected to allow us to significantly improve the constraints derive...
We show that disc continuum fitting can be used to constrain black hole spin in a subclass of narrow...
Using the 770 ks XMM-Newton survey of the Lockman Hole field in combination with extensive optical i...
We discuss black hole spin measurements employing the relativistic iron line profiles in the X-ray d...
Accretion disk reflection spectra, including broad iron emission lines, bear the imprints of the str...
We present an analysis of the observed broad iron line feature and putative warm absorber in the lon...
4 pages, 3 color figures, subm. to ApJWe report on a deep Suzaku observation of the stellar-mass bla...
We fit X-ray spectral data in the thermal dominant or high soft state of two dynamically confirmed b...
The 6.4\,keV Iron reflection line possesses strong diagnostic potential for AGN-systems. In the rare...
Several AGN and black hole X-ray binaries show a clear very broad iron line which is strong evidence...
The micro Seyfert galaxy NGC-4395 hosts a supermassive black hole at its center that actively accret...
International audienceThe interpretation of very broad iron lines in the X-ray spectra of Active Gal...
This dissertation explores the question of whether broad iron lines from the accretion disk can be u...
Recent X-ray spectroscopy made with ASCA have shown broad, skewed iron line emission from Seyfert-1 ...
The Galactic black hole candidate XTE J1752−223 was observed during the decay of its 2009 outburst w...
Future X-ray instrumentation is expected to allow us to significantly improve the constraints derive...
We show that disc continuum fitting can be used to constrain black hole spin in a subclass of narrow...
Using the 770 ks XMM-Newton survey of the Lockman Hole field in combination with extensive optical i...