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Multi-Wavelength Surveys for Galaxies Hidden by the Milky Way

Published online by Cambridge University Press:  12 April 2016

Renée C. Kraan-Korteweg
Renée C. Kraan-Korteweg*
Affiliation:
Departamento de Astronomía, Universidad de Guanajuato, Guanajuato GTO 36000, Mexico

Abstract

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The systematic mapping of obscured and optically invisible galaxies behind the Milky Way through complementary surveys are important in arriving at the whole-sky distribution of complete galaxy samples and therewith for our understanding of the dynamics in the local Universe. In this paper, a status report is given of the various deep optical, near infrared (NIR), and systematic blind H I-surveys in the Zone of Avoidance, including a discussion on the limitations and selection effects inherent to the different multi-wavelength surveys and first results.

Type
Low Surface Brightness galaxy surveys
Information
International Astronomical Union Colloquium , Volume 171: The Low Surface Brightness Universe , 1999 , pp. 103 - 110
Copyright
Copyright © Astronomical Society of the Pacific 1999

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