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- W1660559600 abstract "The ACS grism mode offers an unprecedented opportunity to obtain slitless, highly multiplexed, spectroscopic observations down to very faint magnitudes. In this paper, we show that by selecting objects in a deep field based in the spectra of these objects rather than their broad band colors, a more accurate object selection can be performed. The ACS grism mode enabled us to identify faint, young, and low mass (≈106–108 M⊙) galaxies at 4.0<z<5.7, that are likely to be the building blocks leading to the assembly of the more massive galaxies that we observed in the present universe." @default.
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- W1660559600 date "2009-12-19" @default.
- W1660559600 modified "2023-09-27" @default.
- W1660559600 title "The ACS Grism Mode and ACS Grism Observations of Deep Fields and High z Ly-α Galaxies" @default.
- W1660559600 cites W1994671833 @default.
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- W1660559600 doi "https://doi.org/10.1007/978-90-481-3400-7_42" @default.
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