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Faint galaxy surveys.
Various K band galaxy surveys have now established 2.2-m galaxy counts from K = 10 to K = 23. The K band counts rise slightly faster than a Euclidean slope to K = 17, at which point they turn over; beyond this magnitude, galaxies also become much bluer. Spectroscopic samples are available between K...
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| Main Authors: | , |
|---|---|
| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
1993
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| Teme: | |
| Online dostop: | https://ncbi.nlm.nih.gov/pmc/articles/PMC46614/ https://ncbi.nlm.nih.gov/pubmed/11607401 |
| Oznake: |
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