Multi-Wavelength Surveys for Galaxies Hidden by the Milky Way

Details Multi-Wavelength Surveys for Galaxies Hidden by the Milky Way Multi-Wavelength Surveys for Galaxies Hidden by the Milky Way

1998-10-16

arxiv.org/abs/astro-ph/9810255v1

Astronomy and Astrophysics

Astrophysics

To appear in "The Low Surface Brightness Universe", IAU Coll 171, eds. J.I. Davies et al., A.S.P. Conference Series. 8 pages,

Scientific paper

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 \HI-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.

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