Multi-Wavelength Surveys for Galaxies Hidden by the Milky Way
| dc.creator | Kraan-Korteweg, R. C. | |
| dc.date | 1998-10-16 | |
| dc.date.accessioned | 2026-07-07T02:28:26Z | |
| dc.date.available | 2026-07-07T02:28:26Z | |
| dc.description | 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. | |
| dc.description | To appear in "The Low Surface Brightness Universe", IAU Coll 171, eds. J.I. Davies et al., A.S.P. Conference Series. 8 pages, LaTex, 4 encapsulated ps-figures, requires paspconf.sty | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9810255 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9810255 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/13120 | |
| dc.subject | Astrophysics | |
| dc.title | Multi-Wavelength Surveys for Galaxies Hidden by the Milky Way | |
| dc.type | text |