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- W2140147377 abstract "Abstract Extending the study of star-forming galaxies to z >6 is extremely difficult due to the faintness of the sources and the challenging nature of deep near-infrared observations. Nevertheless, current observations are now just good enough that we can begin drawing some conclusions about the nature of galaxies at z ≳7. At present, deep near-infrared observations with NICMOS (reaching ≳27 AB mag at 5σ) cover more than 20arcmin 2 of area with deep optical coverage and allow us to identify four strong z ≃7–8 candidates. Comparing this sample with dropout samples at later times ( z ≃4–6), we are able to study evolution in the rest-frame UV LF over the range z ≃8 to z ≃4. We find strong evidence for significant evolution in the characteristic luminosity with time (brightening by ∼2 mag, from z ≃8 to z ≃4). The observed evolution appears to be the direct result of hierarchical growth in the galaxy population." @default.
- W2140147377 created "2016-06-24" @default.
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- W2140147377 date "2006-08-01" @default.
- W2140147377 modified "2023-10-14" @default.
- W2140147377 title "Lyman break galaxies at z>6" @default.
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- W2140147377 doi "https://doi.org/10.1017/s1743921307010289" @default.
- W2140147377 hasPublicationYear "2006" @default.
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