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20232026
most citedMeasuring black hole spins with x-ray reflection spectroscopy: A GRMHD outlook

3 citations · 8 across the 13 of their papers we have counts for

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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

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.HE2025

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.HE2025

Assessing the Power-Law Emissivity Assumption in X-ray Reflection Spectroscopy: A Simulation-Based Evaluation of Different Coronal Geometries

Songcheng Li, Abdurakhmon Nosirov, Cosimo Bambi +3

The emissivity profile assumed in X-ray reflection spectroscopy significantly impacts black hole spin measurements. Using simulated NuSTAR spectra generated for lamppost and disk-l…

astro-ph.HE2025★ 3 cited

Measuring black hole spins with x-ray reflection spectroscopy: A GRMHD outlook

Swarnim Shashank, Askar B. Abdikamalov, Honghui Liu +4

X-ray reflection spectroscopy has evolved as one of the leading methods to measure black hole spins. However, the question is whether its measurements are subjected to systematic b…

astro-ph.HE2025

Probing the Strong Gravity Region of Black Holes with eXTP

Qingcui Bu, Cosimo Bambi, Lijun Gou +42

We present the novel capabilities of the enhanced X-ray Timing and Polarimetry (eXTP) mission to study the strong gravity region around stellar-mass black holes in X-ray binary sys…