Catalog Service: Auriga-California Molecular Cloud Catalog
Description
The Auriga-California molecular cloud is a large region of relatively modest star formation that is part of the Gould Belt. The "Auriga-California Molecular Cloud" (ACMC) Herschel program observed a 14.5 square degree area in five far-infrared bands. The ACMC catalog provides photometry for the 60 point-like and very compact sources in each band: PACS 70 and 160 microns, SPIRE 250, 350, and 500 microns.
This section describes who is responsible for this resource
Publisher: NASA/IPAC Infrared Science Archiveivo://irsa.ipac/IRSA[Pub. ID]
Contact Information:
This section provides some status information: the resource version, availability, and relevant dates.
This resource was registered on: 2015 Jan 14 02:45:00ZThis resource description was last updated on: 2018 Oct 01 20:27:20Z
This section describes what the resource is, what it contains, and how it might be relevant.
Related Resources:
This section describes the data's coverage over the sky, frequency, and time.
Wavebands covered:
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.
VERB
This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data.
To access this resource via TAP, issue ADQL queries on the table named acmccat.
This is service that does not comply with any IVOA standard but instead provides access to special capabilities specific to this resource.
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