activity
20172026
most citedA NICER Discovery of a Low-Frequency Quasi-Periodic Oscillation in the Soft-Intermediate State of MAXI J1535-571

44 citations · 123 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2026★ 2 cited

Constraining black hole spin in PG 1535+547 amidst complex multi-layered absorption

A. Madathil-Pottayil, D. J. Walton, Jiachen Jiang +7

We present a spectroscopic analysis of XMM-Newton and NuSTAR observations of the 'complex' NLS1 PG 1535+547 at redshift . These observations span three epochs: 2002 and 20…

astro-ph.HE2026★ 5 cited

Evidence of mutually exclusive outflow forms from a black hole X-ray binary

Zuobin Zhang, Jiachen Jiang, Francesco Carotenuto +13

Accretion onto black holes often leads to the launch of outflows that significantly influence their surrounding environments. The two primary forms of these outflows are X-ray disk…

astro-ph.HE2026★ 1 cited

Decoding Cygnus X-2: The Critical Role of Reflection in IXPE Data

Honghui Liu, Jiachen Jiang, Adam Ingram +10

We present a spectro-polarimetric re-analysis of the first IXPE observation of Cygnus X-2 which we determine to be mainly in the normal branch, from quasi-simultaneous observations…

astro-ph.HE2025★ 1 cited

Non-Equilibrium Thermodynamics of Black-Hole Coronae: QPOs, Turbulence, and Jets

Vanessa López-Barquero, Alejandro Jenkins, Christopher S. Reynolds +1

The variability of X-rays observed from accreting black hole systems, including quasi-periodic oscillations (QPOs), suggests a complex nonlinear dynamics in the corona. Here, we pr…

astro-ph.HE2025★ 6 cited

A rapid black hole spin or emission from the plunging region?

Andrew Mummery, Jiachen Jiang, Adam Ingram +2

Emission from within the plunging region of black hole accretion flows has recently been detected in two X-ray binary systems. There is, furthermore, a possible discrepancy between…

astro-ph.HE2025

NuSTAR observations of a varying-flux quasar in the Epoch of Reionization

Lea Marcotulli, Thomas Connor, Eduardo Bañados +13

With enough X-ray flux to be detected in a 160s scan by SRG/eROSITA, the quasar CFHQS J142952+544717 is, by far, the most luminous X-ray source known at . We pres…

astro-ph.GA2024★ 21 cited

A blazar in the epoch of reionization

Eduardo Banados, Emmanuel Momjian, Thomas Connor +21

Relativistic jets are thought to play a crucial role in the formation and evolution of massive galaxies and supermassive black holes. Blazars, which are quasars with jets aligned a…

astro-ph.HE2024

Plunging region emission in the X-ray binary MAXI J0637430

Andrew Mummery, Jiachen Jiang, Andrew Fabian

On the second of November 2019 the black hole X-ray binary MAXI J0637430 went into outburst, at the start of which it was observed in a thermal ``disc-dominated'' state. High ph…

astro-ph.HE2024

Continuum emission from within the plunging region of black hole discs

Andrew Mummery, Adam Ingram, Shane Davis +1

The thermal continuum emission observed from accreting black holes across X-ray bands has the potential to be leveraged as a powerful probe of the mass and spin of the central blac…

astro-ph.HE2018★ 44 cited

A NICER Discovery of a Low-Frequency Quasi-Periodic Oscillation in the Soft-Intermediate State of MAXI J1535-571

A. L. Stevens, P. Uttley, D. Altamirano +17

We present the discovery of a low-frequency Hz quasi-periodic oscillation (QPO) feature in observations of the black hole X-ray binary MAXI J1535-571 in its soft-inte…

astro-ph.HE2017★ 43 cited

Temperature Structure in the Perseus Cluster Core Observed with Hitomi

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +192

The present paper investigates the temperature structure of the X-ray emitting plasma in the core of the Perseus cluster using the 1.8--20.0 keV data obtained with the Soft X-ray S…