دورية أكاديمية
A high black-hole-to-host mass ratio in a lensed AGN in the early Universe.
| العنوان: | A high black-hole-to-host mass ratio in a lensed AGN in the early Universe. |
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| المؤلفون: | Furtak LJ; Physics Department, Ben-Gurion University of the Negev, Be'er-Sheva, Israel. furtak@post.bgu.ac.il., Labbé I; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Melbourne, Victoria, Australia., Zitrin A; Physics Department, Ben-Gurion University of the Negev, Be'er-Sheva, Israel., Greene JE; Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA., Dayal P; Kapteyn Astronomical Institute, University of Groningen, Groningen, The Netherlands., Chemerynska I; Institut d'Astrophysique de Paris, CNRS, Sorbonne Université, Paris, France., Kokorev V; Kapteyn Astronomical Institute, University of Groningen, Groningen, The Netherlands., Miller TB; Department of Astronomy, Yale University, New Haven, CT, USA.; Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) and Department of Physics and Astronomy, Northwestern University, Evanston, IL, USA., Goulding AD; Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA., de Graaff A; Max-Planck-Institut für Astronomie, Heidelberg, Germany., Bezanson R; Department of Physics and Astronomy and PITT PACC, University of Pittsburgh, Pittsburgh, PA, USA., Brammer GB; Cosmic Dawn Center (DAWN), Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark., Cutler SE; Department of Astronomy, University of Massachusetts, Amherst, MA, USA., Leja J; Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA, USA.; Institute for Computational and Data Sciences, The Pennsylvania State University, University Park, PA, USA.; Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA, USA., Pan R; Department of Physics and Astronomy, Tufts University, Medford, MA, USA., Price SH; Department of Physics and Astronomy and PITT PACC, University of Pittsburgh, Pittsburgh, PA, USA., Wang B; Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA, USA.; Institute for Computational and Data Sciences, The Pennsylvania State University, University Park, PA, USA.; Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA, USA., Weaver JR; Department of Astronomy, University of Massachusetts, Amherst, MA, USA., Whitaker KE; Cosmic Dawn Center (DAWN), Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark.; Department of Astronomy, University of Massachusetts, Amherst, MA, USA., Atek H; Institut d'Astrophysique de Paris, CNRS, Sorbonne Université, Paris, France., Bogdán Á; Center for Astrophysics ∣ Harvard & Smithsonian, Cambridge, MA, USA., Charlot S; Institut d'Astrophysique de Paris, CNRS, Sorbonne Université, Paris, France., Curtis-Lake E; Centre for Astrophysics Research, Department of Physics, Astronomy and Mathematics, University of Hertfordshire, Hatfield, UK., van Dokkum P; Department of Astronomy, Yale University, New Haven, CT, USA., Endsley R; Department of Astronomy, The University of Texas at Austin, Austin, TX, USA., Feldmann R; Institute for Computational Science, University of Zurich, Zurich, Switzerland., Fudamoto Y; Waseda Research Institute for Science and Engineering, Faculty of Science and Engineering, Waseda University, Shinjuku, Tokyo, Japan.; National Astronomical Observatory of Japan, Mitaka, Tokyo, Japan., Fujimoto S; Department of Astronomy, The University of Texas at Austin, Austin, TX, USA., Glazebrook K; Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Melbourne, Victoria, Australia., Juneau S; NSF's National Optical-Infrared Astronomy Research Laboratory, Tucson, AZ, USA., Marchesini D; Department of Physics and Astronomy, Tufts University, Medford, MA, USA., Maseda MV; Department of Astronomy, University of Wisconsin-Madison, Madison, WI, USA., Nelson E; Department for Astrophysical and Planetary Science, University of Colorado, Boulder, CO, USA., Oesch PA; Cosmic Dawn Center (DAWN), Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark.; Department of Astronomy, University of Geneva, Versoix, Switzerland., Plat A; Steward Observatory, University of Arizona, Tucson, AZ, USA., Setton DJ; Department of Physics and Astronomy and PITT PACC, University of Pittsburgh, Pittsburgh, PA, USA., Stark DP; Steward Observatory, University of Arizona, Tucson, AZ, USA., Williams CC; NSF's National Optical-Infrared Astronomy Research Laboratory, Tucson, AZ, USA.; Steward Observatory, University of Arizona, Tucson, AZ, USA. |
| المصدر: | Nature [Nature] 2024 Apr; Vol. 628 (8006), pp. 57-61. Date of Electronic Publication: 2024 Feb 14. |
| نوع المنشور: | Journal Article |
| اللغة: | English |
| بيانات الدورية: | Publisher: Nature Publishing Group Country of Publication: England NLM ID: 0410462 Publication Model: Print-Electronic Cited Medium: Internet ISSN: 1476-4687 (Electronic) Linking ISSN: 00280836 NLM ISO Abbreviation: Nature Subsets: MEDLINE |
| أسماء مطبوعة: | Publication: Basingstoke : Nature Publishing Group Original Publication: London, Macmillan Journals ltd. |
| مواضيع طبية MeSH: | Lens, Crystalline*, Animals ; Dorsal Raphe Nucleus ; Service Animals |
| مستخلص: | Early JWST observations have uncovered a population of red sources that might represent a previously overlooked phase of supermassive black hole growth 1-3 . One of the most intriguing examples is an extremely red, point-like object that was found to be triply imaged by the strong lensing cluster Abell 2744 (ref. 4 ). Here we present deep JWST/NIRSpec observations of this object, Abell2744-QSO1. The spectroscopy confirms that the three images are of the same object, and that it is a highly reddened (A (© 2024. The Author(s), under exclusive licence to Springer Nature Limited.) |
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| تواريخ الأحداث: | Date Created: 20240214 Date Completed: 20240405 Latest Revision: 20240405 |
| رمز التحديث: | 20240405 |
| DOI: | 10.1038/s41586-024-07184-8 |
| PMID: | 38354833 |
| قاعدة البيانات: | MEDLINE |
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Full Text Finder | تدمد: | 1476-4687 |
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| DOI: | 10.1038/s41586-024-07184-8 |