activity
20082023
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 3.5k across the 58 of their papers we have counts for

collaborators

59 papers

astro-ph.HE2023★ 9 cited

The Spin of a Newborn Black Hole: Swift J1728.9-3613

Paul A. Draghis, Mayura Balakrishnan, Jon M. Miller +7

The origin and distribution of stellar-mass black hole spins are a rare window into the progenitor stars and supernova events that create them. Swift J1728.9-3613 is an X-ray binar…

astro-ph.HE2022★ 62 cited

A Systematic View of Ten New Black Hole Spins

Paul A. Draghis, Jon M. Miller, Abderahmen Zoghbi +4

The launch of NuSTAR and the increasing number of binary black hole (BBH) mergers detected through gravitational wave (GW) observations have exponentially advanced our understandin…

astro-ph.HE2021★ 6 cited

A Spectroscopic Angle on Central Engine Size Scales in Accreting Neutron Stars

Nicolas Trueba, J. M. Miller, A. C. Fabian +9

Analyses of absorption from disk winds and atmospheres in accreting compact objects typically treat the central emitting regions in these systems as point sources relative to the a…

astro-ph.GA2021★ 41 cited

Frequency-resolved lags in UV/optical continuum reverberation mapping

Edward M. Cackett, Abderahmen Zoghbi, Otho Ulrich

In recent years, continuum reverberation mapping involving high cadence UV/optical monitoring campaigns of nearby Active Galactic Nuclei has been used to infer the size of their ac…

astro-ph.HE2021

The Spin and Orientation of the Black Hole in XTE J1908094

Paul A. Draghis, Jon M. Miller, Abderahmen Zoghbi +3

NuSTAR observed the black hole candidate XTE J1908094 during its 2013 and 2019 outbursts. We use relativistic reflection to measure the spin of the black hole through 19 differe…

astro-ph.HE2021★ 16 cited

The Inner Accretion Flow in the Resurgent Seyfert-1.2 AGN Mrk 817

J. M. Miller, Z. Zoghbi, M. T. Reynolds +10

Accretion disks and coronae around massive black holes have been studied extensively, and they are known to be coupled. Over a period of 30 years, however, the X-ray (coronal) flux…