activity
20192024
most citedAGN torus detectability at sub-millimeter wavelengths: What to expect from ALMA continuum data

26 citations · 124 across the 10 of their papers we have counts for

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astro-ph.GA2019★ 14 cited

Physical parameters of the torus for the type 2 Seyfert IC 5063 from mid-IR and X-ray simultaneous spectral fitting

Donaji Esparza-Arredondo, Omaira González-Martín, Deborah Dultzin +7

In order to understand the diversity of classes observed in active galactic nuclei (AGN), a geometrically and optically thick torus of gas and dust is required to obscure the centr…

astro-ph.GA2019★ 13 cited

The inner view of NGC 1052 using multiple X-ray observations

Natalia Osorio-Clavijo, Omaira González-Martín, Iossif Papadakis +2

In this paper, we make a multi-epoch analysis of NGC 1052, one of the prototypical LLAGN, using XMM-Newton, Suzaku and NuSTAR observations, taken from 2001 to 2017. This is the fir…

astro-ph.GA2019

Exploring the mid-infrared SEDs of six AGN dusty torus models II: the data

O. González-Martín, J. Masegosa, I. García-Bernete +9

This is the second in a series of papers devoted to explore a set of six dusty models of active galactic nuclei (AGN) with available spectral energy distributions (SEDs). These mod…

astro-ph.GA2019

Exploring the mid-infrared SEDs of six AGN dusty torus models I: synthetic spectra

O. González-Martín, J. Masegosa, I. García-Bernete +9

At distances from the active galaxy nucleus (AGN) where the ambient temperature falls below ~1500-1800 K, dust is able to survive. It is thus possible to have a large dusty structu…

astro-ph.GA2019★ 26 cited

AGN torus detectability at sub-millimeter wavelengths: What to expect from ALMA continuum data

Alice Pasetto, Omaira González-Martín, Donaji Esparza-Arredondo +3

We study the detectability of the emission associated with the AGN dusty structure at sub-mm wavelengths using ALMA, in a theoretical and observational way. Theoretically, we use t…