Catalog Service: NGC1068 MIDI/VLTI observations
Description
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). 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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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2014 May 13 07:48:19ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.
This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data.
This is a standard IVOA service that takes as input a position in the sky and a radius and returns catalog records with positions within that radius.
Cone search capability for table J/A+A/565/A71/list (List of UVFITS file)
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