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Kurt L. Adelberger

Researcher at Google

Publications -  58
Citations -  10901

Kurt L. Adelberger is an academic researcher from Google. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 33, co-authored 58 publications receiving 10732 citations. Previous affiliations of Kurt L. Adelberger include Carnegie Learning & Carnegie Institution for Science.

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Lyman Break Galaxies at z>4 and the Evolution of the UV Luminosity Density at High Redshift

TL;DR: In this paper, the authors present an initial results of a survey for star-forming galaxies in the redshift range 3.8 z 4.5 and z 3.23 deg2 to an apparent magnitude of IAB = 25.0.
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Spectroscopic Confirmation of a Population of Normal Star-forming Galaxies at Redshifts z > 3*

TL;DR: In this paper, the authors reported the discovery of a substantial population of star-forming galaxies at 3.0 z 3.5 and confirmed their existence using deep spectroscopy on the W. M. Keck telescope.
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Lyα Imaging of a Proto-Cluster Region at ⟨z⟩ = 3.09*

TL;DR: In this article, the authors presented very deep narrowband observations of a volume containing a significant overdensity of galaxies previously discovered in a survey for continuum-selected Lyman-break galaxies (LBGs) at redshifts 2.7 z 3.4.
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A Large Structure of Galaxies at Redshift z ~ 3 and Its Cosmological Implications*

TL;DR: In this article, the authors report the discovery of a highly significant concentration of galaxies at a redshift of z = 3.090, which is the first from an ongoing targeted redshift survey designed to explore the nature and distribution of star-forming galaxies in the redshift range 2.7 z 3.4.
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Spectroscopic Confirmation of a Population of Normal Star-Forming Galaxies at Redshifts z>3

TL;DR: Giavalisco et al. as mentioned in this paper reported the discovery of a substantial population of star-forming galaxies at $3.5$ using color criteria sensitive to the presence of a Lyman continuum break superposed on an otherwise very blue far-UV continuum, and confirmed with deep spectroscopy on the W. M. Keck telescope.