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20032023
most citedIntrinsic disc emission and the Soft X-ray Excess in AGN

622 citations · 7.3k across the 65 of their papers we have counts for

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Showing 2011 · astro-ph.HEShow all

6 papers · 2 filters

astro-ph.HE2011★ 622 cited

Intrinsic disc emission and the Soft X-ray Excess in AGN

Chris Done, Shane Davis, Chichuan Jin +2

(Abridged) Narrow Line Seyfert 1 (NLS1) galaxies have low mass black holes and mass accretion rates close to (or exceeding) Eddington, so a standard blackbody accretion disc should…

astro-ph.HE2011★ 267 cited

The Extreme Spin of the Black Hole in Cygnus X-1

Lijun Gou, Jeffrey E. McClintock, Mark J. Reid +7

The compact primary in the X-ray binary Cygnus X-1 was the first black hole to be established via dynamical observations. We have recently determined accurate values for its mass a…

astro-ph.HE2011★ 111 cited

The Cool Accretion Disk in ESO 243-49 HLX-1: Further Evidence of an Intermediate Mass Black Hole

Shane W. Davis, Ramesh Narayan, Yucong Zhu +5

With an inferred bolometric luminosity exceeding 10^42 erg/s, HLX-1 in ESO 243-49 is the most luminous of ultraluminous X-ray sources and provides one of the strongest cases for th…

astro-ph.HE2011★ 61 cited

The X-Ray Polarization Signature of Quiescent Magnetars: Effect of Magnetospheric Scattering and Vacuum Polarization

Rodrigo Fernández, Shane W. Davis

In the magnetar model, the quiescent non-thermal soft X-ray emission from Anomalous X-ray Pulsars and Soft-Gamma Repeaters is thought to arise from resonant comptonization of therm…

astro-ph.HE2011★ 136 cited

Measuring Black Hole Spin by the Continuum-Fitting Method: Effect of Deviations from the Novikov-Thorne Disc Model

Akshay K. Kulkarni, Robert F. Penna, Roman V. Shcherbakov +7

The X-ray spectra of accretion discs of eight stellar-mass black holes have been analyzed to date using the thermal continuum fitting method, and the spectral fits have been used t…

astro-ph.HE2011★ 249 cited

Measuring the Spins of Accreting Black Holes

Jeffrey E. McClintock, Ramesh Narayan, Shane W. Davis +6

A typical galaxy is thought to contain tens of millions of stellar-mass black holes, the collapsed remnants of once massive stars, and a single nuclear supermassive black hole. Bot…