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Title:
Mid-infrared imaging of 25 local AGN with VLT-VISIR
Authors:
Horst, H.; Duschl, W. J.; Gandhi, P.; Smette, A.
Affiliation:
AA(Institut für Theoretische Physik und Astrophysik, Christian-Albrechts-Universität zu Kiel, Leibnizstr. 15, 24098 Kiel, Germany ; Zentrum für Astronomie, ITA, Universität Heidelberg, Albert-Ueberle-Str. 2, 69120 Heidelberg, Germany ; Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany ; European Southern Observatory, Casilla 19001, Santiago 19, Chile), AB(Institut für Theoretische Physik und Astrophysik, Christian-Albrechts-Universität zu Kiel, Leibnizstr. 15, 24098 Kiel, Germany; Steward Observatory, The University of Arizona, 933 N. Cherry Ave, Tucson, AZ 85721, USA), AC(RIKEN Cosmic Radiation Lab, 2-1 Hirosawa, Wakoshi Saitama 351-0198, Japan), AD(European Southern Observatory, Casilla 19001, Santiago 19, Chile)
Publication:
Astronomy and Astrophysics, Volume 495, Issue 1, 2009, pp.137-146 (A&A Homepage)
Publication Date:
02/2009
Origin:
EDP Sciences
DOI:
10.1051/0004-6361:200809878
Bibliographic Code:
2009A&A...495..137H

Abstract

Context: High angular resolution N-band imaging is used to discern the torus of active galactic nuclei (AGN) from its environment in order to allow a comparison of its mid-infrared properties to the expectations of the unified scenario for AGN.
Aims: We present VLT-VISIR images of 25 low-redshift AGN of different Seyfert types, as well as N-band SEDs of 20 of them. In addition, we compare our results for 19 of them to Spitzer IRS spectra.
Methods: We find that at a resolution of 0.35 arcsec, all the nuclei of our observed sources are point-like, except for 2 objects whose extension is likely of instrumental origin. For 3 objects, however, we observed additional extended circumnuclear emission, even though our observational strategy was not designed to detect it. Comparison of the VISIR photometry and Spitzer spectrophotometry indicates that the latter is affected by extended emission in at least 7 out of 19 objects and the level of contamination is (0.20 ˜ 0.85) \cdot FIRS. In particular, the 10 μm silicate emission feature seen in the Spitzer spectra of 6 type I AGN, possibly 1 type II AGN and 2 LINERs, also probably originates not solely in the torus but also in extended regions.
Results: Our results generally agree with the expectations from the unified scenario, while the relative weakness of the silicate feature supports clumpy torus models. Our VISIR data indicate that, for low-redshift AGN, a large fraction of Spitzer IRS spectra are contaminated by extended emission close to the AGN.

Based on ESO observing programmes 075.B-0844(C) and

077.B-0137(A).

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