Catalog Service: Optical counterparts of X-ray sources in OGLE
Description
We present a sample of 209 variable objects - very likely optical counterparts to the X-ray sources detected in the direction of the Galactic center by the Galactic Bulge Survey (GBS) carried out with the Chandra satellite. The variable sources were found in the databases of the OGLE long term survey monitoring regularly the Galactic bulge since 1992. The counterpart candidates were searched based on the X-ray source position in the radius of 3.9 arcsec.
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Publisher: CDSivo://CDS[Pub. ID]
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This resource was registered on: 2013 Feb 08 15:02:18ZThis resource description was last updated on: 2021 Oct 21 00:00:00Z
This section describes what the resource is, what it contains, and how it might be relevant.
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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/AcA/62/133/table2 (Possible bright non-variable optical counterparts to the X-ray sources detected by the Galactic Bulge Survey)
VERB=1
VERB=3
Cone search capability for table J/AcA/62/133/table1 (Optical counterparts to the X-ray sources detected by the Galactic Bulge Survey revealing optical variability)
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