# Investigating the sensitivity of observed spectral energy distributions to clumpy torus properties in Seyfert galaxies

@article{Almeida2014InvestigatingTS,
title={Investigating the sensitivity of observed spectral energy distributions to clumpy torus properties in Seyfert galaxies},
author={Cristina Ramos Almeida and Almudena Alonso-Herrero and N. A. Levenson and A. Asensio Ramos and Jos{\'e} Miguel Rodr{\'i}guez Espinosa and Omaira Gonz{\'a}lez-Mart{\'i}n and Christopher Packham and M. Martinez},
journal={Monthly Notices of the Royal Astronomical Society},
year={2014},
volume={439},
pages={3847-3859}
}
• Published 3 February 2014
• Physics
• Monthly Notices of the Royal Astronomical Society
This research was supported by a Marie Curie Intra European Fellowship within the 7th European Community Framework Programme (PIEF-GA-2012-327934). CRA acknowledges financial support from the Instituto de Astrofisica de Canarias and the Spanish Ministry of Science and Innovation (MICINN) through project PN AYA2010-21887-C04.04 (Estallidos). AAH acknowledges support from the Spanish Plan Nacional de Astronom´ia y Astrofisica under grant AYA2009-05705-E and from the Augusto G. Linares Program…

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## References

SHOWING 1-10 OF 66 REFERENCES
Resolving the nuclear dust distribution of the Seyfert 2 galaxy NGC 3081
• Physics
• 2011
CRA acknowledges financial support from STFC (ST/G001758/1) and from the Spanish Ministry of Science and Innovation (MICINN) through project Consolider-Ingenio 2010 Programme grant CSD2006-00070:
Testing the Unification Model for Active Galactic Nuclei in the Infrared: Are the Obscuring Tori of Type 1 and 2 Seyferts Different?
• Physics
• 2011
We present new mid-infrared (MIR) imaging data for three Type-1 Seyfert galaxies obtained with T-ReCS on the Gemini-South Telescope at subarcsecond resolution. Our aim is to enlarge the sample
Probing the nuclear and circumnuclear activity of NGC 1365 in the infrared
• Environmental Science
• 2012
This development has been supported by the funding agencies BMVIT (Austria), ESA-PRODEX (Belgium), CEA/CNES (France), DLR (Germany), ASI/INAF (Italy) and CICYT/MCYT (Spain). SPIRE has been developed
THE INFRARED NUCLEAR EMISSION OF SEYFERT GALAXIES ON PARSEC SCALES: TESTING THE CLUMPY TORUS MODELS
• Physics
• 2009
We present subarcsecond resolution mid-infrared (mid-IR) photometry in the range from 8 to 20 μm of 18 nearby Seyfert galaxies, reporting high spatial resolution nuclear fluxes for the entire sample
Modeling the Nuclear Infrared Spectral Energy Distribution of Type II Active Galactic Nuclei
• Physics
• 2013
We present results from model fitting to the spectral energy distribution (SED) of a homogeneous sample of Seyfert II galaxies drawn from the 12 μm Galaxy Sample. Imaging and nuclear flux
Uncovering the Deeply Embedded Active Galactic Nucleus Activity in the Nuclear Regions of the Interacting Galaxy Arp 299
• Physics
• 2013
We present mid-infrared (MIR) 8-13 μm spectroscopy of the nuclear regions of the interacting galaxy Arp 299 (IC 694+NGC 3690) obtained with CanariCam (CC) on the 10.4 m Gran Telescopio Canarias
Resolving the mid-infrared cores of local Seyferts
• Physics
• 2009
We present new photometry of 16 local Seyferts including 6 Compton-thick sources in N -band filters around 12- μ m, obtained with the VISIR instrument on the 8-m Very Large Telescope. The
The innermost region of AGN tori: implications from the HST/NICMOS type 1 point sources and near-IR reverberation
• Physics, Geology
• 2007
Spatially resolving the innermost region of the putative torus-like structure in an active galactic nucleus (AGN) is one of the main goals of high-spatial-resolution studies. This could be done in
The effect of stellar feedback on the formation and evolution of gas and dust tori in AGN
• Physics
• 2009
Recently, the existence of geometrically thick dust structures in active galactic nuclei (AGN) has been directly proven with the help of interferometric methods in the mid-infrared. The observations
Dust in active galactic nuclei. Mid-infrared T-ReCS/Gemini spectra using the new RedCan pipeline
• Physics
• 2012
Context. The unified model of active galactic nuclei (AGN) claims that the properties of AGN depend on the viewing angle of the observer with respect to a toroidal distribution of dust surrounding