activity
20182021
most citedThe hot dust in the heart of NGC 1068's torus: A 3D radiative model constrained with GRAVITY/VLTi

10 citations · 12 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.GA202110 cited

The hot dust in the heart of NGC 1068's torus: A 3D radiative model constrained with GRAVITY/VLTi

Pierre Vermot, Yann Clénet, Damien Gratadour +5

The central region of NGC 1068 is one of the closest and most studied Active Galactic Nucleus. It is known to be of type 2, meaning that its accretion disk is obscured by a large a…

astro-ph.GA20212 cited

High angular resolution polarimetric imaging of the nucleus of NGC 1068: Disentangling the polarising mechanisms

L. Grosset, D. Rouan, F. Marin +8

Polarisation is a decisive method to study the inner region of active galactic nuclei (AGNs) since it is not affected by contrast issues similarly to how classical imaging is. When…

astro-ph.HE2019

The role of Active Galactic Nuclei in galaxy evolution: insights from space ultraviolet spectropolarimetry

F. Marin, S. Charlot, B. Agís González +6

This Astro2020 white paper summarizes the unknowns of active galactic nuclei (AGN) physics that could be unveiled thanks to a new, space-born, ultraviolet spectropolarimeter. The u…

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.GA2018

Stellar cusp and warm dust at the heart of NGC1068

Daniel Rouan, Lucas Grosset, Damien Gratadour

Establishing precisely how stars and interstellar medium distribute within the central 100 pc area around an AGN, down to the pc scale, is key for understanding how the very final…