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- W1924311918 abstract "We present the results of detailed surface photometry of a sample of early-type galaxies in the Hubble Deep Field (HDF). Effective radii, surface brightnesses, and total V606 magnitudes have been obtained, as well as U300, B450, I814, J, H, and K colors, which are compared with the predictions of chemical spectrophotometric models of population synthesis. Spectroscopic redshifts are available for 23 objects. For the other 25, photometric redshifts are given. In the ⟨μe⟩-re plane, the early-type galaxies of the HDF turn out to follow the rest frame Kormendy relation once the appropriate K- and evolutionary corrections are applied. This evidence, linked to the dynamical information gathered by Steidel et al., indicates that these galaxies, even at z ≃ 2–3, lie in the fundamental plane in a virial equilibrium condition. At the same redshifts a statistically significant lack of large galaxies (i.e., with log r > 0.2) is observed." @default.
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- W1924311918 date "1998-04-01" @default.
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- W1924311918 title "Early-Type Galaxies in the Hubble Deep Field: The [FORMULA][F][angl0]μ[INF]e[/INF][angr0]-r[INF]e[/INF][/F][/FORMULA] Relation and the Lack of Large Galaxies at High Redshift" @default.
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- W1924311918 doi "https://doi.org/10.1086/300280" @default.
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