3D-HST: A Spectroscopic Galaxy Evolution Treasury Part 2

Details 3D-HST: A Spectroscopic Galaxy Evolution Treasury Part 2 3D-HST: A Spectroscopic Galaxy Evolution Treasury Part 2

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009hst..prop12328v&link_type=abstract

HST Proposal ID #12328. Cycle 18

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Scientific paper

The Hubble Space Telescope has given us a dazzling imaging legacy, which has enabled us to establish a broad picture across cosmic epochs of how galaxies came to be. Here we propose to extend this legacy with 3D-HST, a peerless near-IR spectroscopic program for studying the physical processes that shape galaxies in the distant Universe. Ground-based optical spectroscopy has provided redshifts of large numbers of UV-bright Lyman break galaxies, but they make up only a fraction of the general galaxy population at z>1. 3D-HST will provide rest-frame optical spectra for a complete sample of ~9000 galaxies at 1

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