Erratum: “The Small Sizes and High Implied Densities of “Little Red Dots” with Balmer Breaks Could Explain Their Broad Emission Lines without an Active Galactic Nucleus” (2024, ApJL, 977, L13)

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Main Authors: Josephine F. W. Baggen, Pieter van Dokkum, Gabriel Brammer, Anna de Graaff, Marijn Franx, Jenny Greene, Ivo Labbé, Joel Leja, Michael V. Maseda, Erica J. Nelson, Hans-Walter Rix, Bingjie Wang, Andrea Weibel
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
Online Access:https://doi.org/10.3847/2041-8213/adb424
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author Josephine F. W. Baggen
Pieter van Dokkum
Gabriel Brammer
Anna de Graaff
Marijn Franx
Jenny Greene
Ivo Labbé
Joel Leja
Michael V. Maseda
Erica J. Nelson
Hans-Walter Rix
Bingjie Wang
Andrea Weibel
author_facet Josephine F. W. Baggen
Pieter van Dokkum
Gabriel Brammer
Anna de Graaff
Marijn Franx
Jenny Greene
Ivo Labbé
Joel Leja
Michael V. Maseda
Erica J. Nelson
Hans-Walter Rix
Bingjie Wang
Andrea Weibel
author_sort Josephine F. W. Baggen
collection DOAJ
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id doaj-art-dd30456843ae4fa28b4ca98e4cfd7a70
institution OA Journals
issn 2041-8205
language English
publishDate 2025-01-01
publisher IOP Publishing
record_format Article
series The Astrophysical Journal Letters
spelling doaj-art-dd30456843ae4fa28b4ca98e4cfd7a702025-08-20T02:14:28ZengIOP PublishingThe Astrophysical Journal Letters2041-82052025-01-019802L4710.3847/2041-8213/adb424Erratum: “The Small Sizes and High Implied Densities of “Little Red Dots” with Balmer Breaks Could Explain Their Broad Emission Lines without an Active Galactic Nucleus” (2024, ApJL, 977, L13)Josephine F. W. Baggen0https://orcid.org/0009-0005-2295-7246Pieter van Dokkum1https://orcid.org/0000-0002-8282-9888Gabriel Brammer2https://orcid.org/0000-0003-2680-005XAnna de Graaff3https://orcid.org/0000-0002-2380-9801Marijn Franx4https://orcid.org/0000-0002-8871-3026Jenny Greene5https://orcid.org/0000-0002-5612-3427Ivo Labbé6https://orcid.org/0000-0002-2057-5376Joel Leja7https://orcid.org/0000-0001-6755-1315Michael V. Maseda8https://orcid.org/0000-0003-0695-4414Erica J. Nelson9https://orcid.org/0000-0002-7524-374XHans-Walter Rix10https://orcid.org/0000-0003-4996-9069Bingjie Wang11https://orcid.org/0000-0001-9269-5046Andrea Weibel12https://orcid.org/0000-0001-8928-4465Department of Astronomy, Yale University , New Haven, CT 06511, USA ; josephine.baggen@yale.eduDepartment of Astronomy, Yale University , New Haven, CT 06511, USA ; josephine.baggen@yale.eduCosmic Dawn Center (DAWN), Niels Bohr Institute, University of Copenhagen , Jagtvej 128, København N, DK-2200, DenmarkMax-Planck-Institut für Astronomie , Königstuhl 17, D-69117, Heidelberg, GermanyLeiden Observatory, Leiden University , P.O. Box 9513, NL-2300 RA Leiden, The NetherlandsDepartment of Astrophysical Sciences, Princeton University , 4 Ivy Lane, Princeton, NJ 08544, USACentre for Astrophysics and Supercomputing, Swinburne University of Technology , Melbourne, VIC 3122, AustraliaDepartment of Astronomy & Astrophysics, The Pennsylvania State University , University Park, PA 16802, USA; Institute for Computational & Data Sciences, The Pennsylvania State University , University Park, PA 16802, USA; Institute for Gravitation and the Cosmos, The Pennsylvania State University , University Park, PA 16802, USADepartment of Astronomy, University of Wisconsin-Madison , 475 N. Charter Street, Madison, WI 53706, USADepartment for Astrophysical and Planetary Science, University of Colorado , Boulder, CO, USAMax-Planck-Institut für Astronomie , Königstuhl 17, D-69117, Heidelberg, GermanyDepartment of Astronomy & Astrophysics, The Pennsylvania State University , University Park, PA 16802, USA; Institute for Computational & Data Sciences, The Pennsylvania State University , University Park, PA 16802, USA; Institute for Gravitation and the Cosmos, The Pennsylvania State University , University Park, PA 16802, USADepartment of Astronomy, University of Geneva , Chemin Pegasi 51, 1290 Versoix, Switzerlandhttps://doi.org/10.3847/2041-8213/adb424
spellingShingle Josephine F. W. Baggen
Pieter van Dokkum
Gabriel Brammer
Anna de Graaff
Marijn Franx
Jenny Greene
Ivo Labbé
Joel Leja
Michael V. Maseda
Erica J. Nelson
Hans-Walter Rix
Bingjie Wang
Andrea Weibel
Erratum: “The Small Sizes and High Implied Densities of “Little Red Dots” with Balmer Breaks Could Explain Their Broad Emission Lines without an Active Galactic Nucleus” (2024, ApJL, 977, L13)
The Astrophysical Journal Letters
title Erratum: “The Small Sizes and High Implied Densities of “Little Red Dots” with Balmer Breaks Could Explain Their Broad Emission Lines without an Active Galactic Nucleus” (2024, ApJL, 977, L13)
title_full Erratum: “The Small Sizes and High Implied Densities of “Little Red Dots” with Balmer Breaks Could Explain Their Broad Emission Lines without an Active Galactic Nucleus” (2024, ApJL, 977, L13)
title_fullStr Erratum: “The Small Sizes and High Implied Densities of “Little Red Dots” with Balmer Breaks Could Explain Their Broad Emission Lines without an Active Galactic Nucleus” (2024, ApJL, 977, L13)
title_full_unstemmed Erratum: “The Small Sizes and High Implied Densities of “Little Red Dots” with Balmer Breaks Could Explain Their Broad Emission Lines without an Active Galactic Nucleus” (2024, ApJL, 977, L13)
title_short Erratum: “The Small Sizes and High Implied Densities of “Little Red Dots” with Balmer Breaks Could Explain Their Broad Emission Lines without an Active Galactic Nucleus” (2024, ApJL, 977, L13)
title_sort erratum the small sizes and high implied densities of little red dots with balmer breaks could explain their broad emission lines without an active galactic nucleus 2024 apjl 977 l13
url https://doi.org/10.3847/2041-8213/adb424
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