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Erratum: “2 mm Observations and the Search for High-redshift Dusty Star-forming Galaxies” (2023, ApJ, 952, 28)

The Astrophysical journal, 2024-01, Vol.960 (1), p.92

2024

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Candidate z ∼ 2.5 Lyman Continuum Sources in the GOODS Fields

The Astrophysical journal, 2021-02, Vol.908 (2), p.222

2021

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z ∼ 2.5-3 Ionizers in the GOODS-N Field

The Astrophysical journal, 2018-08, Vol.862 (2), p.142

2018

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The history of star formation in the universe

Contemporary physics, 2017-04, Vol.58 (2), p.160-175

Barger, A. J.

2017

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Resolving the extragalactic hard X-ray background

Nature (London), 2000-03, Vol.404 (6777), p.459-464

2000

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The OPTX Project. II. Hard X-Ray Luminosity Functions of Active Galactic Nuclei for z 5

The Astrophysical journal, 2009-06, Vol.698 (1), p.380-396

2009

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Submillimetre-wavelength detection of dusty star-forming galaxies at high redshift

Nature (London), 1998-07, Vol.394 (6690), p.248-251

1998

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A FLUX-LIMITED SAMPLE OF z ∼ 1 Lyα EMITTING GALAXIES IN THE CHANDRA DEEP FIELD SOUTH

The Astrophysical journal, 2012-04, Vol.749 (2), p.1-13

2012

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THE FAINTEST X-RAY SOURCES FROM z = 0 TO 8

The Astrophysical journal, 2012-03, Vol.748 (1), p.50

2012

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Erratum: “The Evolution of the Ultraluminous Lyα Luminosity Function over z = 5.7–6.6” (2021, ApJ, 914, 79)

The Astrophysical journal, 2022-08, Vol.935 (1), p.63

2022

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Synthetic Statistical Approach Reveals a High Degree of Richness of Microbial Eukaryotes in an Anoxic Water Column

Applied and Environmental Microbiology, 2006-10, Vol.72 (10), p.6578-6583

2006

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A parametric model for the distribution of the angle of arrival and the associated correlation function and power spectrum at the mobile station

IEEE transactions on vehicular technology, 2002-05, Vol.51 (3), p.425-434

2002

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The Number Density of Intermediate- and High-Luminosity Active Galactic Nuclei at z ~ 2-3

The Astrophysical journal, 2005-12, Vol.635 (1), p.115-122

2005

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Tracing activity in distant supermassive black holes with X-rays

Contemporary physics, 2002-09, Vol.43 (5), p.339-349

Barger, A. J.

2002

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The submillimetre extragalactic background light and the star–formation history of the Universe

Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences, 2000-07, Vol.358 (1772), p.2133-2141

2000

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The Nature of the Bright Submillimeter Galaxy Population: A Radio-preselected Sample with I > ~25

The Astrophysical journal, 2001-02, Vol.548 (2), p.L147-L151

2001

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The Ultraluminous Ly Luminosity Function at z = 6.6

The Astrophysical journal, 2020-06, Vol.895 (2)

2020

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LUMINOSITY DEPENDENCE AND REDSHIFT EVOLUTION OF STRONG EMISSION-LINE DIAGNOSTICS IN STAR-FORMING GALAXIES Based in part on data obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA and was made possible by the generous financial support of the W. M. Keck Foundation

The Astrophysical journal, 2016-01, Vol.817 (1)

2016

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Complex Ly Profiles in Redshift 6.6 Ultraluminous Ly Emitters Based on data collected at the Subaru Telescope, which is operated by the National Astronomical Observatory of Japan. † † The W. M. Keck Observatory is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA and was made possible by the generous financial support of the W. M. Keck Foundation

The Astrophysical journal, 2018-05, Vol.859 (2)

2018

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A SUBMILLIMETER PERSPECTIVE ON THE GOODS FIELDS. II. THE HIGH RADIO POWER POPULATION IN THE GOODS-N The James Clerk Maxwell Telescope is operated by the East Asian Observatory on behalf of The National Astronomical Observatory of Japan, Academia Sinica Institute of Astronomy and Astrophysics, the Korea Astronomy and Space Science Institute, the National Astronomical Observatories of China, and the Chinese Academy of Sciences (grant No. XDB09000000), with additional funding support from the Scien

The Astrophysical journal, 2017-01, Vol.835 (1)

2017

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A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). I. An Ultradeep SCUBA-2 Survey of the GOODS-N The James Clerk Maxwell Telescope is operated by the East Asian Observatory on behalf of The National Astronomical Observatory of Japan, Academia Sinica Institute of Astronomy and Astrophysics, the Korea Astronomy and Space Science Institute, the National Astronomical Observatories of China and the Chinese Academy of Sciences (Grant No. XDB09000000), with additional funding support from t

The Astrophysical journal, 2017-03, Vol.837 (2)

2017

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THE OPTX PROJECT. V. IDENTIFYING DISTANT ACTIVE GALACTIC NUCLEI

The Astrophysical journal, 2011-11, Vol.742 (1)

2011

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PRECISE IDENTIFICATIONS OF SUBMILLIMETER GALAXIES: MEASURING THE HISTORY OF MASSIVE STAR-FORMING GALAXIES TO z > 5

The Astrophysical journal, 2012-12, Vol.761 (2), p.89

2012

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A FLUX-LIMITED SAMPLE OF z {approx} 1 Ly{alpha} EMITTING GALAXIES IN THE CHANDRA DEEP FIELD SOUTH

The Astrophysical journal, 2012-04, Vol.749 (2)

2012

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