activity
20242026
collaborators

6 papers

astro-ph.HE2026

Testing General Relativity with NuSTAR data of Galactic Black Holes : II

Ashutosh Tripathi, Swarnim Shashank, Gitika Mall +1

General relativity predicts the spacetime metric around an astrophysical black hole to be described by the Kerr solution, which is a massive rotating black hole without any residua…

astro-ph.HE2025

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

Modeling reflection spectra of super-Eddington X-ray sources

Swarnim Shashank, Askar B. Abdikamalov, Honghui Liu +5

Relativistic reflection is a common feature in the X-ray observations of accreting compact objects. We present reflux, a new X-ray reflection model for spectral analysis of super-E…

astro-ph.HE2025

Testing Regular Black Holes with X-ray data of GX 339-4

Shafqat Riaz, Michail Kyriazis, Askar B. Abdikamalov +2

Regular black holes are singularity-free black hole spacetimes proposed to solve the problem of the presence of spacetime singularities that plagues the black holes of general rela…

astro-ph.HE2024

About the accuracy of the relxill/relxill_nk models in view of the next generation of X-ray missions

Honghui Liu, Askar B. Abdikamalov, Temurbek Mirzaev +4

X-ray reflection spectroscopy is a powerful tool to study the strong gravity region of black holes. The next generation of astrophysical X-ray missions promises to provide unpreced…

astro-ph.HE2024

X-ray spectra of black hole X-ray binaries with returning radiation

Temurbek Mirzaev, Cosimo Bambi, Askar B. Abdikamalov +4

In the disk-corona model, the X-ray spectrum of a stellar-mass black hole in an X-ray binary is characterized by three components: a thermal component from a thin and cold accretio…