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Table · dataset · 2014

NGC1068 MIDI/VLTI observations

Listed in IVOA Registry (Virtual Observatory)

The aim of this paper is to understand the relation in active galactic nuclei (AGNs) between the small obscuring torus and dusty structures at larger scales (5-10pc).

Description

The dusty structures in AGNs are best observed in the mid-infrared. To achieve the necessary spatial resolution (20-100 milliarcsec) we use ESO's Mid-Infrared Interferometer (MIDI) with the 1.8m Auxiliary Telescopes.

We use the chromatic phases in the data to improve the spatial fidelity of the analysis.

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Documentation and papers

Catalogue records · 2

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Inferred from text
Astronomical sciences 72%
Provenance · 1 source records, 8 field assertions
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/565/a7114 d agoJSON v1
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concepts[field].anzsrc:group:5101enrichment · IVOA Registrytaxonomy-embedding@1.1.0title+keywords+description (72%)
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
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license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
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updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0