NGC1068 MIDI/VLTI observations

DOI

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.

Cone search capability for table J/A+A/565/A71/list (List of UVFITS file)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35650071
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/565/A71
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/565/A71
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/565/A71
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/565/A71
Provenance
Creator Lopez-Gonzaga N.; Jaffe W.; Burtscher L.; Tristram K.R.W.; Meisenheimer K.
Publisher CDS
Publication Year 2014
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; High Energy Astrophysics; Natural Sciences; Observational Astronomy; Physics