Matthew P. Hunt

TL;DR: In this paper, the authors presented the first results of a large-scale survey of star-forming galaxies, carried out with the blue channel of the LRIS spectrograph (LRIS-B) on the Keck I Telescope.

TL;DR: In this article, the first results of a large-scale survey, using the UV/blue sensitive LRIS-B spectrograph on the Keck I telescope, of galaxies in the redshift interval 1.4 =2.34 were presented.

TL;DR: In this paper, a detailed study of the interstellar medium (ISM) of MS 1512-cB58, an ~L* Lyman break galaxy at z = 2.7276, based on new spectral observations obtained with the Echelle Spectrograph and Imager on the Keck II telescope at 58 km s-1 resolution.

TL;DR: In this article, the authors present simple and efficient strategies that can be used to find large numbers of galaxies throughout this important but unexplored redshift range, which are based on selecting galaxies for spectroscopy on the basis of their colors in ground-based images taken through a small number of optical filters.

TL;DR: In this article, the authors present simple and efficient strategies that can be used to find large numbers of galaxies throughout this important but unexplored redshift range, which is based on selecting galaxies for spectroscopy on the basis of their colors in ground-based images taken through a small number of optical filters: GRi for redshifts 0.851.5, and UGR for 1.4