UBV Photoelectric Sequences in SA 92-115

The UBV system was originally defined by ten bright standard stars, primarily in the northern sky. These stars are too bright to be used with large telescopes and cannot be reached from southern observatories. This catalog is a careful compilation of data on fainter stars in the equatorial Selected Areas. They are intended as a new set of standards which can be used to define the UBV system at fainter magnitudes in both hemispheres. The stars range in V between 6.0 and 14.9 with most between 9.0 and 13.0.

Cone search capability for table VI/19/gicfeige (Photoelectric Photometry of Giclas, Feige Stars)

Cone search capability for table VI/19/selstars (Selected Area Stars)

Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/VI/19
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/VI/19
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=VI/19
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/VI/19
Creator Landolt A.U.
Publisher CDS
Publication Year 1997
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Resource Type Dataset
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics