STOKES tables and KY codes
astro-ph.HE
Submitted: 2026-08-31
Updated: 2026-10-23
Comments: Invited chapter for the edited book "X-ray Polarimetry: Detection, Observations, Modeling and the Future" (Eds. Honghui Liu and Adam Ingram), Springer Singapore, expected in 2026
Code: https://github.com/jpodgorny/stokes_tables
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- An extended scheme for fitting X-ray data with accretion disk spectra in the strong gravity regime
- Thermal disc emission from a rotating black hole: X-ray polarization signatures
- Light bending scenario for accreting black holes in X-ray polarimetry
- An XSPEC model to explore spectral features from black-hole sources - II. The relativistic iron line in the lamp-post geometry
- Spectral and polarization properties of black hole accretion disc emission: including absorption effects
- A physical model for the broadband energy spectrum of X-ray illuminated accretion discs: fitting the spectral energy distribution of NGC 5548
- Spectral and polarization properties of reflected X-ray emission from black-hole accretion discs for a distant observer: the lamp-post model
- Polarization properties of thermal accretion disk emission. I. Direct radiation
- Spectral and polarization properties of reflected X-ray emission from black hole accretion discs
- X-ray Polarization of the Black Hole X-ray Binary 4U 1630-47 Challenges Standard Thin Accretion Disk Scenario
- Shape and ionization of equatorial matter near compact objects from X-ray polarization reflection signatures
- X-ray polarization of reflected thermal emission
- Escape probability methods versus "exact" transfer for modelling the X-ray spectrum of Active Galactic Nuclei and X-ray binaries
- The 2025 Release of Cloudy
- Modeling optical and UV polarization of AGNs I. Imprints of individual scattering regions
- Modeling optical and UV polarization of AGNs II. Polarization imaging and complex reprocessing
- Modeling optical and UV polarization of AGNs III. From uniform-density to clumpy regions
- Modeling optical and UV polarization of AGNs V. Dilution by interstellar polarization and the host galaxy
- X-ray reflected spectra from accretion disk models. I. Constant density atmospheres
- The structure and radiation spectra of illuminated accretion discs in AGN. I. Moderate illumination
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