RefleX provides a flexible Monte Carlo code for X-ray reprocessing in quasi-arbitrary geometries around AGN, validated against pexrav/MYTorus/BNTorus, with released RXTorus torus model showing bound-electron effects on NGC 424 fits.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
fields
astro-ph.HE 3representative citing papers
Multi-mission X-ray imaging and spectroscopy of the PWN around PSR B1853+01 reveals a hard-spectrum outflow and diffuse halo interpreted as escaping high-energy particles.
Flux-resolved NuSTAR spectra of 4U 0115+63 show the 10 keV feature maintains constant centroid energy while its flux ratio to the continuum anticorrelates with overall flux, indicating a formation mechanism distinct from both the broadband continuum and the CRSF harmonics.
citing papers explorer
-
RefleX: X-ray absorption and reflection in active galactic nuclei for arbitrary geometries
RefleX provides a flexible Monte Carlo code for X-ray reprocessing in quasi-arbitrary geometries around AGN, validated against pexrav/MYTorus/BNTorus, with released RXTorus torus model showing bound-electron effects on NGC 424 fits.
-
The pulsar wind nebula around B1853+01 in X-rays
Multi-mission X-ray imaging and spectroscopy of the PWN around PSR B1853+01 reveals a hard-spectrum outflow and diffuse halo interpreted as escaping high-energy particles.
-
Flux variability of the "10 keV feature" of 4U 0115+63
Flux-resolved NuSTAR spectra of 4U 0115+63 show the 10 keV feature maintains constant centroid energy while its flux ratio to the continuum anticorrelates with overall flux, indicating a formation mechanism distinct from both the broadband continuum and the CRSF harmonics.