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Lyman Break Galaxies at z~3 and Beyond

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arxiv astro-ph/9812167 v1 pith:7R6QB5BV submitted 1998-12-09 astro-ph

C.C. Steidel (1) , K.L. Adelberger (1) , M. Dickinson (2) , M. Giavalisco (2) , M. Pettini (3) ((1) Palomar Observatory , Caltech (2) STScI (3) IoA , Cambridge) This is my paper · ORCID
classification astro-ph
keywords breakgalaxiesluminositylymanstaradvantagesbeyondclustering
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We report on the status of large surveys of photometrically selected star forming galaxies at z~3 and z~4, with particular emphasis on both the advantages and the limitations of selecting objects using the ``Lyman break'' technique. Current results on the luminosity functions, luminosity densities, color distribution, star formation rates, clustering properties, and the differential evolution of the population as a function of redshift are summarized.

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  1. Lyman Break Galaxy selection and redshift measurement with supervised contrastive learning

    astro-ph.CO 2026-08 conditional novelty 6.0 of 10

    A supervised weighted contrastive learning pipeline, zlbg, improves contaminant rejection in DESI Lyman Break Galaxy spectra while matching the redshift accuracy of the existing lbgNET pipeline.

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