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Broad Iron Emission from Gravitationally Lensed Quasars Observed by Chandra
D. J. Walton, M. T. Reynolds, J. M. Miller +3
Recent work has demonstrated the potential of gravitationally lensed quasars to extend measurements of black hole spin out to high-redshift with the current generation of X-ray obs…
ASTRO-H White Paper - Stellar-Mass Black Holes
J. M. Miller, S. Mineshige, A. Kubota +10
Thanks to extensive observations with X-ray missions and facilities working in other wavelengths, as well as rapidly--advancing numerical simulations of accretion flows, our knowle…
A Rapidly Spinning Black Hole Powers the Einstein Cross
Mark T. Reynolds, Dominic J. Walton, Jon M. Miller +1
Observations over the past 20 years have revealed a strong relationship between the properties of the supermassive black hole (SMBH) lying at the center of a galaxy and the host ga…
The Quiescent X-ray Spectrum of Accreting Black Holes
Mark T. Reynolds, Rubens C. Reis, Jon M. Miller +2
The quiescent state is the dominant accretion mode for black holes on all mass scales. Our knowledge of the X-ray spectrum is limited due to the characteristic low luminosity in th…
Reflection From the Strong Gravity Regime in a z=0.658 Gravitationally Lensed-Quasar
Rubens C. Reis, Mark T. Reynolds, Jon M. Miller +1
The co-evolution of a supermassive black hole with its host galaxy through cosmic time is encoded in its spin. At , supermassive black holes are thought to grow mostly by merg…
Multi-Wavelength Coverage of State Transitions in the New Black Hole X-Ray Binary Swift J1910.2-0546
N. Degenaar, D. Maitra, E. M. Cackett +11
Understanding how black holes accrete and supply feedback to their environment is one of the outstanding challenges of modern astrophysics. Swift J1910.2-0546 is a candidate black…