Galaxies and large scale structure at high redshifts
It is now straightforward to assemble large samples of very high redshift (z ∼ 3) field galaxies selected by their pronounced spectral discontinuity at the rest frame Lyman limit of hydrogen (at 912 Å). This makes possible both statistical analyses of the properties of the galaxies and the first dir...
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| Publicado no: | Proc Natl Acad Sci U S A |
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| Autor principal: | |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
National Academy of Sciences
1998
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.govhttps://pmc.ncbi.nlm.nih.gov/articles/PMC34185/ https://ncbi.nlm.nih.govhttps://pubmed.ncbi.nlm.nih.gov/9419319/ https://ncbi.nlm.nih.govhttps://doi.org/10.1073/pnas.95.1.22 |
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