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Article
The corona contracts in a black-hole transient
The geometry of the accretion flow around stellar-mass black holes can change on timescales of days to months1–3. When a black hole emerges from quiescence (that is, it ‘turns on’ after accreting material from it...
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Article
X-ray reverberation around accreting black holes
Luminous accreting stellar mass and supermassive black holes produce power–law continuum X-ray emission from a compact central corona. Reverberation time lags occur due to light travel time delays between chan...
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Article
The Large Observatory for X-ray Timing (LOFT)
High-time-resolution X-ray observations of compact objects provide direct access to strong-field gravity, to the equation of state of ultradense matter and to black hole masses and spins. A 10 m2-class instrument...
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Article
Broad line emission from iron K- and L-shell transitions in the active galaxy 1H 0707-495
The emission line arising from a transition of an electron from the iron K shell to the ground state (the K line) is prominent in the reflection spectrum of the hard X-ray continuum irradiating dense accreting...
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Chapter and Conference Paper
AGN and XRB Variability: Propagating-Fluctuation Models
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Article
Active galactic nuclei as scaled-up Galactic black holes
The central engines that drive active galactic nuclei are thought to be supermassive black holes. A long-standing question in astrophysics is whether these central engines vary like Galactic black hole systems...