activity
20072026
most citedSpectral and temporal properties of Compton scattering by mildly relativistic thermal electrons

163 citations · 658 across the 42 of their papers we have counts for

collaborators

43 papers

astro-ph.HE2026

Model dependence of XRISM black-hole spin constraints in Cyg X-1

Andrzej A. Zdziarski, Swadesh Chand, Michal Szanecki +2

We study the persistent black hole X-ray binary Cyg X-1, recently observed by XRISM Resolve and simultaneously by NICER and NuSTAR in its hard spectral state. We confirm the result…

astro-ph.HE2026

X-ray polarization in the soft state of Cyg X-1

A. Niedzwiecki, M. Szanecki, A. Veledina +5

We aim to identify the physical mechanism responsible for the observed X-ray emission and polarization of Cyg X-1 in the soft state. We performed a detailed spectral analysis of X-…

astro-ph.HE2025

The strong Fe K line and spin of the black-hole X-ray binary MAXI J1631-479

Andrzej A. Zdziarski, Swadesh Chand, Gulab Dewangan +5

We study the transient black hole binary MAXI J1631--479 in its soft spectral state observed simultaneously by the NICER and NuSTAR instruments. Its puzzling feature is the presenc…

astro-ph.HE2024★ 1 cited

Is the Spin of the Black Hole in GX 339-4 Negative?

Andrzej A. Zdziarski, Srimanta Banerjee, Michal Szanecki +2

We have studied the accreting black hole binary GX 339--4 using two highly accurate broad-band X-ray data sets in very soft spectral states from simultaneous NICER and NuSTAR obser…

astro-ph.HE2024

Broad band spectral modeling of M87 nucleus

Andrzej Niedzwiecki, Michal Szanecki, Agnieszka Janiuk

We study spectra produced by weakly accreting black hole (BH) systems using the semi-analytic advection dominated accretion flow (ADAF) model and the general-relativistic magentohy…

astro-ph.HE2024

What Is the Black Hole Spin in Cyg X-1?

Andrzej A. Zdziarski, Swadesh Chand, Srimanta Banerjee +6

We perform a detailed study of the black hole spin of Cyg X-1, using accurate broad-band X-ray data obtained in the soft spectral state by simultaneous NICER and NuSTAR observation…