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Jul 29, 2024 | 
nature.com | Stefano Carniani |Daniel Eisenstein |Peter Viggo Jakobsen |Benjamin Johnson |Roberto Maiolino |Chris Willott | +24 more
AbstractThe first observations of JWST have revolutionized our understanding of the Universe by identifying for the first time galaxies at \(z\sim 13\)1–3. In addition, the discovery of many luminous galaxies at Cosmic Dawn (\(z > 10\)) has suggested that galaxies developed rapidly, in apparent tension with many standard models4–8. However, most of these galaxies lack spectroscopic confirmation, so their distances and properties are uncertain.
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Jul 29, 2024 | nature.com | Stefano Carniani |Daniel Eisenstein |Peter Viggo Jakobsen |Benjamin Johnson |Roberto Maiolino |Chris Willott | +24 more
AbstractThe first observations of JWST have revolutionized our understanding of the Universe by identifying for the first time galaxies at \(z\sim 13\)1–3. In addition, the discovery of many luminous galaxies at Cosmic Dawn (\(z > 10\)) has suggested that galaxies developed rapidly, in apparent tension with many standard models4–8. However, most of these galaxies lack spectroscopic confirmation, so their distances and properties are uncertain.
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Jul 29, 2024 | nature.com | Stefano Carniani |Daniel Eisenstein |Peter Viggo Jakobsen |Benjamin Johnson |Roberto Maiolino |Chris Willott | +24 more
AbstractThe first observations of JWST have revolutionized our understanding of the Universe by identifying for the first time galaxies at \(z\sim 13\)1–3. In addition, the discovery of many luminous galaxies at Cosmic Dawn (\(z > 10\)) has suggested that galaxies developed rapidly, in apparent tension with many standard models4–8. However, most of these galaxies lack spectroscopic confirmation, so their distances and properties are uncertain.
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Apr 19, 2024 | 
hal.science | Eleonora Parlanti |Stefano Carniani |Hannah Übler |Giacomo Venturi
Article Dans Une Revue Astronomy and Astrophysics - A&A Année : 2024 GA-NIFS: Early-stage feedback in a heavily obscured AGN at $z=4.76$ Origine : Fichiers éditeurs autorisés sur une archive ouverte hal-04230073 , version 1 (19-04-2024) Eleonora Parlanti, Stefano Carniani, Hannah Übler, Giacomo Venturi, Francesco d'Eugenio, et al.. GA-NIFS: Early-stage feedback in a heavily obscured AGN at $z=4.76$.
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Mar 29, 2024 | 
aanda.org | Stefano Carniani |Hannah Übler |Madingley Road |Eleonora Parlanti
Home All issues Volume 684 (April 2024) A&A, 684 (2024) A24 Full HTML Issue A&A Volume 684, April 2024 Article Number A24 Number of page(s) 23 Section Extragalactic astronomy DOI https://doi.org/10.1051/0004-6361/202347914 Published online 29 March 2024 A&A, 684, A24 (2024) GA-NIFS: Early-stage feedback in a heavily obscured active galactic nucleus at z = 4.76 1, 1, 2,3, 1, 4,5, 2,3, 6, 7, 8, 9, 2,3,5, 6, 6, 10, 9, 7, 7, 11, 7, 12, 6 and 2,3 1 Scuola Normale Superiore, Piazza dei Cavalieri 7,...
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Feb 12, 2024 | 
aanda.org | Gareth Jones |Denys Wilkinson Building |Keble Road |Hannah Übler
Home All issues Volume 682 (February 2024) A&A, 682 (2024) A122 Full HTML Issue A&A Volume 682, February 2024 Article Number A122 Number of page(s) 23 Section Extragalactic astronomy DOI https://doi.org/10.1051/0004-6361/202347838 Published online 12 February 2024 A&A 682, A122 (2024) GA-NIFS: JWST/NIRSpec integral field unit observations of HFLS3 reveal a dense galaxy group at z ∼ 6.3 1, 2,3, 4, 4, 1, 5, 6, 2,3,7, 4, 8, 9, 10, 1, 1, 11, 12, 2,3, 13, 1,7, 2,3, 5 and 2,3 1 Department of...
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Jan 17, 2024 | 
nature.com | Roberto Maiolino |Joris Witstok |Stefano Carniani |Anna de Graaff |Hannah Übler |Sandro Tacchella | +20 more
AbstractMultiple theories have been proposed to describe the formation of black hole seeds in the early Universe and to explain the emergence of very massive black holes observed in the first billion years after Big Bang1–3. Models consider different seeding and accretion scenarios4–7, which require the detection and characterisation of black holes in the first few hundred million years after Big Bang to be validated.
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Jan 17, 2024 | nature.com | Roberto Maiolino |Joris Witstok |Stefano Carniani |Anna de Graaff |Hannah Übler |Sandro Tacchella | +20 more
AbstractMultiple theories have been proposed to describe the formation of black hole seeds in the early Universe and to explain the emergence of very massive black holes observed in the first billion years after Big Bang1–3. Models consider different seeding and accretion scenarios4–7, which require the detection and characterisation of black holes in the first few hundred million years after Big Bang to be validated.
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Jan 17, 2024 | nature.com | Roberto Maiolino |Joris Witstok |Stefano Carniani |Anna de Graaff |Hannah Übler |Sandro Tacchella | +20 more
AbstractMultiple theories have been proposed to describe the formation of black hole seeds in the early Universe and to explain the emergence of very massive black holes observed in the first billion years after Big Bang1–3. Models consider different seeding and accretion scenarios4–7, which require the detection and characterisation of black holes in the first few hundred million years after Big Bang to be validated.
