collaborators

15 papers

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

Dense, multi-phase accretion disk atmosphere in the low-luminosity state of black hole transientV4641 Sgr

Zuobin Zhang, Rob Fender, James H. Matthews +11

We present soft X-ray spectroscopy of the black-hole X-ray binary V4641~Sgr with the \textit{XMM-Newton} Reflection Grating Spectrometer (RGS). The RGS spectrum shows narrow emissi…

astro-ph.HE2026

Assessing systematic uncertainties from spectral re-analysis of Cyg X-1 with different coronal geometries

Abdurakhmon Nosirov, Jiachen Jiang, Cosimo Bambi +1

In this work, we carry out a new spectral reanalysis of NuSTAR and Suzaku observations of the disk reflection spectra in the stellar-mass black hole X-ray binary Cyg~X-1. We compar…

astro-ph.HE2026

Searching for Isolated Black Hole Candidates within 15 pc of the Solar System in Gaia DR3

Abdurakhmon Nosirov, Cosimo Bambi, Leda Gao +4

Theoretical models predict that the Galaxy hosts - black holes formed from the complete gravitational collapse of heavy stars and that most of these black holes are iso…

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

DAO: A New and Public Non-Relativistic Reflection Model

Yimin Huang, Honghui Liu, Cosimo Bambi +4

We present a new non-relativistic reflection model, DAO, designed to calculate reflection spectra in the rest frame of accretion disks in X-ray binaries and active galactic nuclei.…