Add to ORKGpeer reviewedThe optical polarization properties of both low- and high-luminosity active galactic nuclei (AGN) are described, focusing on the origin of the polarization and its relation to the AGN structure, in particular the geometry of the scattering regions. State-of-the-art modeling, polarization reverberation and microlensing, as well as the polarization of changing-look AGNs will be discussed
peer reviewedOptical polarization signal coming from the innermost part of active galactic nuclei (A...
I review the optical polarization properties of both low- and high-luminosity AGN, focusing on the ...
We present results from a new Monte Carlo radiative transfer computer code, STOKES, developed to mod...
The optical polarization properties of both low- and high-luminosity active galactic nuclei (AGN) a...
The anisotropic nature of active galactic nuclei (AGN) is thought to be responsible for the observat...
Among all the astronomical sources investigated through the prism of polarimetry, active galactic nu...
Context. Spectropolarimetry of AGNs is a powerful tool for studying the structure and kinematics of ...
International audienceAn important unknown for Seyfert Galaxies is the exact geometry and nature of ...
Context. Spectropolarimetry of AGNs is a powerful tool for studying the structure and kinematics of ...
International audienceContext. One of the main challenges for polarimetric observations of active ga...
International audienceContext: Spectropolarimetry of AGNs is a powerful tool for studying the struct...
Context. One of the main challenges for polarimetric observations of active galactic nuclei (AGN) is...
International audienceIn this second research note of a series of two, we present the first near-inf...
The unified model for AGN stats that Seyfert 1 or 2 types are the same type of object harbouring a l...
International audienceContext. Optical observations cannot resolve the structure of active galactic ...
peer reviewedOptical polarization signal coming from the innermost part of active galactic nuclei (A...
I review the optical polarization properties of both low- and high-luminosity AGN, focusing on the ...
We present results from a new Monte Carlo radiative transfer computer code, STOKES, developed to mod...
The optical polarization properties of both low- and high-luminosity active galactic nuclei (AGN) a...
The anisotropic nature of active galactic nuclei (AGN) is thought to be responsible for the observat...
Among all the astronomical sources investigated through the prism of polarimetry, active galactic nu...
Context. Spectropolarimetry of AGNs is a powerful tool for studying the structure and kinematics of ...
International audienceAn important unknown for Seyfert Galaxies is the exact geometry and nature of ...
Context. Spectropolarimetry of AGNs is a powerful tool for studying the structure and kinematics of ...
International audienceContext. One of the main challenges for polarimetric observations of active ga...
International audienceContext: Spectropolarimetry of AGNs is a powerful tool for studying the struct...
Context. One of the main challenges for polarimetric observations of active galactic nuclei (AGN) is...
International audienceIn this second research note of a series of two, we present the first near-inf...
The unified model for AGN stats that Seyfert 1 or 2 types are the same type of object harbouring a l...
International audienceContext. Optical observations cannot resolve the structure of active galactic ...
peer reviewedOptical polarization signal coming from the innermost part of active galactic nuclei (A...
I review the optical polarization properties of both low- and high-luminosity AGN, focusing on the ...
We present results from a new Monte Carlo radiative transfer computer code, STOKES, developed to mod...