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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 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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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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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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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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THE FAINTEST X-RAY SOURCES FROM z = 0TO8

The Astrophysical journal, 2012-03, Vol.748 (1), p.1-12

2012

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THE HOST GALAXIES OF X-RAY QUASARS ARE NOT STRONG STAR FORMERS, The James Clerk Maxwell Telescope has historically been operated by the Joint Astronomy Centre on behalf of the Science and Technology Facilities Council of the United Kingdom, the National Research Council of Canada and The Netherlands Organisation for Scientific Research. Additional funds for the construction of SCUBA-2 were provided by the Canada Foundation for Innovation. , The National Radio Astronomy Observatory is a facility

The Astrophysical journal, 2015-03, Vol.801 (2)

2015

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AN ULTRALUMINOUS LY EMITTER WITH A BLUE WING AT z = 6.6 ∗ 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

Astrophysical journal. Letters, 2016-06, Vol.825 (1)

2016

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The Redshift Evolution of the 2–8 [CLC]ke[/CLC]V X-Ray Luminosity Function

The Astrophysical journal, 2003-02, Vol.584 (2), p.L57-L60

2003

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Supermassive Black Hole Accretion History Inferred from a Large Sample of [ITAL]CHANDRA[/ITAL][ITAL]Chandra[/ITAL] Hard X-Ray Sources

The Astronomical journal, 2001-11, Vol.122 (5), p.2177-2189

2001

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The cosmic history of the X-ray background: One contribution of 13 to a Discussion Meeting `The impact of active galaxies on the Universe at large

Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences, 2005-03, Vol.363 (1828), p.685-694

Barger, A J

2005

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AN ATLAS OF z = 5.7 AND z = 6.5 Ly{alpha} EMITTERS

The Astrophysical journal, 2010-12, Vol.725 (1)

2010

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