Abstract
Obvious targets for Extremely Large Telescopes are high-redshift galaxies and galaxy (proto-)clusters. However, due to the extremely small field-of-view of such telescopes, finding such objects, notably the rarer proto-clusters, is best be done using other facilities. The very helpful negative K-correction experienced in the far-IR to mm wavebands makes surveys in these wavebands the ideal pathfinders for high-z ELT targets.
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CITATION STYLE
APA
Kampen, E. V. (2009). The first galaxies and galaxy clusters. In Astrophysics and Space Science Proceedings (Vol. 0, pp. 183–185). Springer Science and Business Media B.V. https://doi.org/10.1007/978-1-4020-9190-2_31
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