activity
20122025
most citedModeling optical and UV polarization of AGNs II. Polarization imaging and complex reprocessing

83 citations · 248 across the 12 of their papers we have counts for

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Showing astro-ph.HEShow all

9 papers · 1 filter

astro-ph.HE2018★ 3 cited

A near-infrared, optical and ultraviolet polarimetric and timing investigation of complex equatorial dusty structures

F. Marin, P. A. Rojas Lobos, J. M. Hameury +1

Context. From stars to active galactic nuclei, many astrophysical systems are surrounded by an equatorial distribution of dusty material that are, in a number of cases, spatially u…

astro-ph.HE2017★ 38 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.HE2017★ 23 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★ 22 cited

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.HE2015★ 62 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…

astro-ph.HE2013

Dust in the wind I: spectropolarimetric signatures from disk-born outflows

F. Marin, R. W. Goosmann

In this first research note of a series of two, we conduct optical/UV investigations of the spectropolarimetric signatures emerging from the structure of quasars (Elvis 2000) appli…

astro-ph.HE2012

UV and optical polarization modeling of thermal active galactic nuclei : impact of the narrow line region

F. Marin, R. W. Goosmann

In this research note, we start exploring the influence of the narrow line region (NLR) on the optical/UV continuum polarization of active galactic nuclei (AGN). We have upgraded o…

astro-ph.HE2012★ 83 cited

Modeling optical and UV polarization of AGNs II. Polarization imaging and complex reprocessing

F. Marin, R. W. Goosmann, C. M. Gaskell +2

We model the spectropolarimetric signature resulting from the radiative coupling between the innermost parts of active galactic nuclei (AGNs). We use a new public version of STOKES…

astro-ph.HE2012★ 16 cited

X-ray polarimetry as a new tool to discriminate reflection from absorption scenarios -- Predictions for MCG-6-30-15

F. Marin, R. W. Goosmann, M. Dovciak +5

We present modelling of X-ray polarisation spectra emerging from the two competing scenarios that are proposed to explain the broad Fe Kα line in the Seyfert 1 galaxy MCG-6-30-15.…