activity
20242026
most citedThe 2018 outburst of MAXI J1820+070 as seen by Insight-HXMT

7 citations · 22 across the 13 of their papers we have counts for

collaborators

15 papers

astro-ph.IM2026

EXPO: a quantum leap in fast, wide-band X-ray polarimetry for astrophysics

Paolo Soffitta, Sebastien Guillot, Ian Hutchinson +137

The Enhanced X-ray Polarimetry Observatory (EXPO) is a mission concept proposed to ESA as an M8 candidate, with a prospective launch in 2041. Building on the scientific success of…

astro-ph.HE2026

Radio flares and X-ray hardening embedded in the long soft state of 4U 1543-475

Zuobin Zhang, Rob Fender, Jiachen Jiang +14

We present a comprehensive multi-wavelength study of the black hole X-ray binary 4U 1543-475 during its 2021 outburst, focusing on radio flaring episodes that are commonly interpre…

astro-ph.HE2026

Black-Hole Spin Measurements from X-ray Reflection Spectroscopy: Quality Criteria and Community Recommendations

Javier A. Garcia, Riley Connors, Laura W. Brenneman +1

X-ray reflection spectroscopy provides one of the most powerful electromagnetic methods for measuring the dimensionless spin of accreting black holes. It has yielded spin constrain…

astro-ph.HE2026

Spin Demographics of Active Supermassive Black Holes: Updated Estimates from X-ray reflection and Future opportunities

Julia M. Sisk-Reynes, Christopher S. Reynolds, James H. Matthews +5

Understanding the growth of supermassive black holes (SMBHs) requires observational constraints on how their angular momentum (or spin) varies with mass, since the relative importa…

astro-ph.HE2026

Systematic assessment of disk truncation in the black hole X-ray binary Swift J1727.8-1613 using NICER

Ole König, James F. Steiner, Niek Bollemeijer +20

The 2023/24 NICER monitoring campaign of the 7 Crab bright black hole X-ray binary Swift J1727.8-1613 covered the outburst in almost all accretion states. High-quality data are ava…

astro-ph.HE2026

Exploring the spin dependence on mass inclination and distance for the newly discovered black hole X-ray binary Swift J151857.0-572147

Yujia Song, James F. Steiner, Tong Zhao +7

The black hole X-ray binary (BHXRB) Swift J151857.0-572147 was discovered during its first outburst in March 2024. We review the archive of NICER observations from this outburst, f…

astro-ph.HE2026

A clean broad iron line in GS 1354--64 as seen by XRISM

Honghui Liu, Lingda Kong, Oluwashina K. Adegoke +13

We present a spectroscopic analysis of XRISM and NuSTAR observations of the black hole X-ray binary GS~1354--64 during its 2026 outburst. A total number of 3.5 million photons are…

astro-ph.HE2026

Discovery of Strong Energy-Dependent X-ray Polarization in the Intermediate State of GS 1354-64

Swati Ravi, Lorenzo Marra, James F. Steiner +20

We report the discovery of significant X-ray polarization from the dynamically confirmed black hole X-ray binary (BHXB) GS 1354-64 during its 2025-2026 outburst, obtained with the…

astro-ph.HE2026

A NICER view of the corona through time-dependent Comptonization of the quasi-periodic oscillations in nine black-hole X-ray binaries

Yuexin Zhang, Mariano Méndez, James F. Steiner +12

We present a systematic study of the evolution of the corona geometry in nine black hole X-ray binaries (BHXRBs) using archival data from NICER. We identify 171 observations exhibi…

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.HE2025★ 2 cited

Possible Coronal Geometry in the Hard and Soft State of Black Hole X-ray Binaries from MONK Simulations

Ningyue Fan, Cosimo Bambi, James F. Steiner +1

Understanding the coronal geometry in different states of black hole X-ray binaries is important for more accurate modeling of the system. However, it is difficult to distinguish d…

astro-ph.HE2025★ 2 cited

Constraining Disk-to-Corona Power Transfer Fraction, Soft X-ray Excess Origin, and Black Hole Spin Population of Type-1 AGN across Mass Scales

Labani Mallick, Ciro Pinto, John Tomsick +6

Understanding the nature of the accretion disk, its interplay with the X-ray corona, and assessing black hole spin demographics remain open challenges in astrophysics. In this pape…

astro-ph.HE2024★ 1 cited

NICER Spectral and Timing Analysis of 4U 163047 and its Heartbeat State

Ningyue Fan, James F. Steiner, Cosimo Bambi +3

We present a spectral and timing analysis of NICER observations of the black hole X-ray binary 4U 1630-47 from 2018 to 2024. We find relativistic reflection features in the hard an…

astro-ph.HE2024★ 7 cited

The 2018 outburst of MAXI J1820+070 as seen by Insight-HXMT

Ningyue Fan, Songyu Li, Rui Zhan +8

We present an analysis of the whole 2018 outburst of the black hole X-ray binary MAXI J1820+070 with Insight-HXMT data. We focus our study on the temporal evolution of the paramete…

astro-ph.HE2024★ 5 cited

Impact of reflection Comptonization on X-ray reflection spectroscopy: the case of EXO 1846-031

Songcheng Li, Honghui Liu, Cosimo Bambi +2

Within the disk-corona model, it is natural to expect that a fraction of reflection photons from the disk are Compton scattered by the hot corona (reflection Comptonization), even…