activity
20172022
most citedReverberation Reveals the Truncated Disc in the Hard State of GX 339-4

61 citations · 184 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2022★ 8 cited

Origins of the UV/X-ray Relation in Arakelian 120

Ra'ad David Mahmoud, Chris Done, Delphine Porquet +1

We explore the accretion geometry in Arakelian 120 using intensive UV and X-ray monitoring from \textit{Swift}. The hard X-rays ( keV) show large amplitude, fast (few-day) va…

astro-ph.HE2020★ 21 cited

Looking for the underlying cause of black hole X-ray variability in GRMHD simulations

D. A. Bollimpalli, R. Mahmoud, C. Done +4

Long-term observations have shown that black hole X-ray binaries exhibit strong, aperiodic variability on time-scales of a few milliseconds to seconds. The observed light curves di…

astro-ph.HE2019★ 22 cited

Discarding the disc in a changing state AGN: the UV/X-ray relation in NGC 4151

Ra'ad D. Mahmoud, Chris Done

Recent monitoring campaigns designed to map the accretion regime in AGN show major discrepancies with models where the optical/ultraviolet (UV) is produced by X-ray-illuminated, op…

astro-ph.HE2018★ 61 cited

Reverberation Reveals the Truncated Disc in the Hard State of GX 339-4

Ra'ad D. Mahmoud, Chris Done, Barbara De Marco

The nature and geometry of the hard state in black hole binaries is controversial. The broadband continuum spectrum and fast variability properties can be explained in a model wher…

astro-ph.HE2018★ 47 cited

A Physical Model for the Spectral-Timing Properties of Accreting Black Holes

Ra'ad D. Mahmoud, Chris Done

We develop new techniques to deconvolve the radial structure of the X-ray emission region in the bright low/hard state of the black hole Cygnus X-1 using both spectral and timing d…

astro-ph.HE2017★ 25 cited

Modelling the Energy Dependence of Black Hole Binary Flows

Ra'ad D. Mahmoud, Chris Done

We build a full spectral-timing model for the low/hard state of black hole binaries assuming that the spectrum of the X-ray hot flow can be produced by two Comptonisation zones. Sl…