Catalog Service: UBVRI photometry in Be 15, Be 80 and NGC 2192
Description
The three open clusters Be 15, Be 80 and NGC 2192 have been observed using CCD UBV(RI)C photometry at the San Pedro Martir Observatory, Mexico within the framework of our open-cluster survey. The fundamental parameters of interstellar reddening, distance and age have been derived, and also the metallicity for NGC 2192 (solar metallicity has been assumed for the other two).
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2010 Jul 10 20:11:43ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
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This section describes the data's coverage over the sky, frequency, and time.
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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/MNRAS/401/621/table1 (Standard UBVRI CCD photometry and observing errors for the open cluster Be 15)
VERB=1
VERB=3
Cone search capability for table J/MNRAS/401/621/table2 (Standard UBVRI CCD photometry and observing errors for the open cluster for Be 80)
Cone search capability for table J/MNRAS/401/621/table3 (Standard UBVRI CCD photometry and observing errors for the open cluster for NGC 2192)
Developed with the support of the National Science Foundation under Cooperative Agreement AST0122449 with the Johns Hopkins University The NAVO project is a member of the International Virtual Observatory Alliance
This NAVO Application is hosted by the Space Telescope Science Institute