Auriga-California Molecular Cloud Catalog Virtual Observatory Resource

Authors

1. Harvey et al. (2013)

Published by

NASA/IPAC Infrared Science Archive

Abstract

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.

Keywords

1. star formation

See also HTML

https://irsa.ipac.caltech.edu/data/Herschel/ACMC/gator_docs/acmc_colDescriptions.html

IVOA Identifier IVOID

ivo://irsa.ipac/Herschel/Catalog/ACMC

Access

IVOA Cone Search SCS

For use with a cone search client (e.g., TOPCAT).
https://irsa.ipac.caltech.edu/SCS?table=acmccat&

IVOA Table Access TAP

https://irsa.ipac.caltech.edu/TAP
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

Web browser access HTML

https://irsa.ipac.caltech.edu/cgi-bin/Gator/nph-dd?catalog=acmccat