ESO VLTI Calibrators Program

DOI

The ESO Very Large Telescope Interferometer (VLTI) is one of the leading interferometric facilities. It is equiped with several 8.2 and 1.8m telescopes, a large number of baselines up to 200m, and with several subsystems designed to enable high quality measurements and to improve significantly the limits of sensitivities currently available to long-baseline interferometry. For this, a large number of observations of potential calibrators have been obtained during the commissioning phase of the VLTI. These data are publicly available.

Cone search capability for table J/A+A/434/1201/table4 (Candidate VLTI calibrators)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34341201
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/434/1201
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/434/1201
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/434/1201
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/434/1201
Provenance
Creator Richichi A.; Percheron I.
Publisher CDS
Publication Year 2005
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; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy