activity
20122019
most citedModeling optical and UV polarization of AGNs III. From uniform-density to clumpy regions

62 citations · 123 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2019

The panchromatic polarization signatures of Active Galactic Nuclei

F. Marin

Among all the astronomical sources investigated through the prism of polarimetry, active galactic nuclei (AGN) have proven to be the richest in terms of complex yet fundamental sig…

astro-ph.IM2018

Probing the structure and evolution of active galactic nuclei with the ultraviolet polarimeter POLLUX aboard LUVOIR

F. Marin, S. Charlot, D. Hutsemékers +6

The ultraviolet (UV) polarization spectrum of nearby active galactic nuclei (AGN) is poorly known. The Wisconsin Ultraviolet Photo-Polarimeter Experiment and a handful of instrumen…

astro-ph.HE201738 cited

Predicting the X-ray polarization of type-2 Seyfert galaxies

F. Marin, M. Dovciak, F. Muleri +2

Infrared, optical and ultraviolet spectropolarimetric observations have proven to be ideal tools for the study of the hidden nuclei of type-2 active galactic nuclei (AGN) and for c…

astro-ph.HE201723 cited

Unveiling the physics behind the spectral variations of "changing-look" quasars with optical polarimetry

F. Marin

A handful of active galactic nuclei (AGN) have shown strong spectral variations in the optical band between epochs that are years apart. The appearance or disappearance of broad em…

astro-ph.HE2016

X-ray polarimetric signatures induced by spectral variability in the framework of the receding torus model

F. Marin, R. W. Goosmann, P. -O. Petrucci

Obscuring circumnuclear dust is a well-established constituent of active galactic nuclei (AGN). Traditionally referred to as the receding dusty torus, its inner radius and angular…

astro-ph.HE201562 cited

Modeling optical and UV polarization of AGNs III. From uniform-density to clumpy regions

F. Marin, R. W. Goosmann, C. M. Gaskell

A growing body of evidence suggests that part of, if not all, scattering regions of active galactic nuclei (AGNs) are clumpy. Hence. in this paper, we run radiative transfer models…