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The NOAO Variable-Sky Project

Published online by Cambridge University Press:  20 April 2012

T. Matheson
Affiliation:
National Optical Astronomy Observatory, Tucson, AZ 85719, USA email: [email protected]
R. Blum
Affiliation:
National Optical Astronomy Observatory, Tucson, AZ 85719, USA email: [email protected]
B. Jannuzi
Affiliation:
National Optical Astronomy Observatory, Tucson, AZ 85719, USA email: [email protected]
T. Lauer
Affiliation:
National Optical Astronomy Observatory, Tucson, AZ 85719, USA email: [email protected]
D. Norman
Affiliation:
National Optical Astronomy Observatory, Tucson, AZ 85719, USA email: [email protected]
K. Olsen
Affiliation:
National Optical Astronomy Observatory, Tucson, AZ 85719, USA email: [email protected]
S. Ridgway
Affiliation:
National Optical Astronomy Observatory, Tucson, AZ 85719, USA email: [email protected]
A. Saha
Affiliation:
National Optical Astronomy Observatory, Tucson, AZ 85719, USA email: [email protected]
R. Shaw
Affiliation:
National Optical Astronomy Observatory, Tucson, AZ 85719, USA email: [email protected]
A. Walker
Affiliation:
National Optical Astronomy Observatory, Tucson, AZ 85719, USA email: [email protected]
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Abstract

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Modern time-domain surveys have demonstrated that finding variable objects is relatively straightforward. The problem now is one of selecting and following up discoveries. With even larger-scale surveys on the horizon, the magnitude of the problem will inevitably increase. One way to prepare for the coming deluge is to have realistic estimates of the numbers of potential detections so that resources can be developed to meet that need. To that end, astronomers at the National Optical Astronomy Observatory (NOAO) have begun a project to characterize the variable sky in terms of type of objects, distribution on the sky and range of variation.

Keywords

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

References

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