Catalog Service: Chandra sources in ONC & BN-KL
Description
About 1000 X-ray emitting young premain-sequence (PMS) stars distributed in mass from ~0.05M_{sun}_ brown dwarfs to a ~50M_{sun}_ O star are detected in an image of the Orion Nebula obtained with the Advanced CCD Imaging Spectrometer (ACIS) on board the Chandra X-Ray Observatory. The sources in the Becklin-Neugebauer/Kleinman-Low region of massive star formation are discussed in detail.
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Publisher: CDSivo://CDS[Pub. ID]
Contact Information:
This section provides some status information: the resource version, availability, and relevant dates.
This resource was registered on: 2001 May 11 15:42:31ZThis 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.
Wavebands covered:
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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/AJ/120/1426/table1 (ACIS sources in the ONC)
VERB=1
VERB=3
Cone search capability for table J/AJ/120/1426/table2 (ACIS sources near the Becklin-Neugebauer (BN) object)
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