The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z ∼ 8

被引：0

作者：

Curti, Mirko ^{[1
,2
]}

D’Eugenio, Francesco ^{[1
,2
]}

Carniani, Stefano ^{[3
]}

Maiolino, Roberto ^{[1
,2
,4
]}

Sandles, Lester ^{[1
,2
]}

Witstok, Joris ^{[1
,2
]}

Baker, William M. ^{[1
,2
]}

Bennett, Jake S. ^{[1
,5
]}

Piotrowska, Joanna M. ^{[1
,2
]}

Tacchella, Sandro ^{[1
,2
]}

Charlot, Stephane ^{[6
]}

Nakajima, Kimihiko ^{[7
]}

Maheson, Gabriel ^{[1
,2
]}

Mannucci, Filippo ^{[8
]}

Amiri, Amirnezam ^{[8
,9
]}

Arribas, Santiago ^{[10
]}

Belfiore, Francesco ^{[8
]}

Bonaventura, Nina R. ^{[11
]}

Bunker, Andrew J. ^{[12
]}

Chevallard, Jacopo ^{[12
]}

Cresci, Giovanni ^{[8
]}

Curtis-Lake, Emma ^{[13
]}

Hayden-Pawson, Connor ^{[1
,2
]}

Jones, Gareth C. ^{[12
]}

Kumari, Nimisha ^{[14
]}

Laseter, Isaac ^{[15
]}

Looser, Tobias J. ^{[1
,2
]}

Marconi, Alessandro ^{[8
,9
]}

Maseda, Michael V. ^{[15
]}

Scholtz, Jan ^{[1
,2
]}

Smit, Renske ^{[16
]}

Übler, Hannah ^{[1
,2
]}

Wallace, Imaan E.B. ^{[12
]}

机构：

[1] Kavli Institute for Cosmology, University of Cambridge, Madingley Road, Cambridge,CB3 0HA, United Kingdom

[2] Cavendish Laboratory, Astrophysics Group, University of Cambridge, 19 JJ Thompson Avenue, Cambridge,CB3 0HE, United Kingdom

[3] Scuola Normale Superiore, Università di Pisa, Piazza dei Cavalieri 7, Pisa,I-56126, Italy

[4] Department of Physics and Astronomy, University College London, Gower Street, London,WC1E 6BT, United Kingdom

[5] Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge,CB3 0HA, United Kingdom

[6] Sorbonne Université, UPMC-CNRS, UMR7095, Institut d’Astrophysique de Paris, Paris,F-75014, France

[7] National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo,181-8588, Japan

[8] INAF — Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, Florence,I-50125, Italy

[9] Dipartimento di Fisica e Astronomia, Universitá di Firenze, Via G. Sansone 1, Sesto Fiorentino, Florence,I-50125, Italy

[10] Centro de Astrobiología (CAB), CSIC–INTA, Cra. de Ajalvir Km. 4, Torrejón de Ardoz, Madrid,28850, Spain

[11] Cosmic Dawn Center, Niels Bohr Institute, University of Copenhagen, Rådmandsgade 62, Copenhagen N,2200, Denmark

[12] Department of Physics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford,OX13RH, United Kingdom

[13] Centre for Astrophysics Research, Department of Physics, Astronomy and Mathematics, University of Hertfordshire, Hatfield,AL10 9AB, United Kingdom

[14] AURA for the European Space Agency, Space Telescope Science Institute, 3700 San Martin Drive, Baltimore,MD,21218, United States

[15] Department of Astronomy, University of Wisconsin-Madison, 475 N. Charter St., Madison,WI,53706, United States

[16] Astrophysics Research Institute, Liverpool John Moores University, 146 Brownlow Hill, Liverpool,L3 5RF, United Kingdom

来源：

arXiv | 2022年

关键词：

Compendex;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

Galaxies

引用

共 28 条

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[22] Early Results from GLASS-JWST. XVIII. A First Morphological Atlas of the 1 < z < 5 Universe in the Rest-frame Optical
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Treu, T.
Nannayakkara, T.
Jones, T.
Merlin, E.
Abraham, R.
Stevens, A. R. H.
Vulcani, B.
Yang, L.
Bonchi, A.
Boyett, K.
Bradac, M.
Castellano, M.
Fontana, A.
Marchesini, D.
Malkan, M.
Mason, C.
Morishita, T.
Paris, D.
Santini, P.
Trenti, M.
Wang, X.
ASTROPHYSICAL JOURNAL LETTERS, 2023, 948 (02)
[23] UV luminosity density results at z > 8 from the first JWST/NIRCam fields: limitations of early data sets and the need for spectroscopy
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[24] High-z Universe Probed via Lensing by QSOs (HULQ). I. Number Estimates of QSO-QSO and QSO-Galaxy Lenses
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[25] JWST Identification of Extremely Low C/N Galaxies with [N/O] ≳ 0.5 at z ∼ 6-10 Evidencing the Early CNO-cycle Enrichment and a Connection with Globular Cluster Formation
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[27] 3-cm FINE STRUCTURE MASERS: A UNIQUE SIGNATURE OF SUPERMASSIVE BLACK HOLE FORMATION VIA DIRECT COLLAPSE IN THE EARLY UNIVERSE
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[28] EMPRESS. XIII. Chemical Enrichment of Young Galaxies Near and Far at z ∼ 0 and 4-10: Fe/O, Ar/O, S/O, and N/O Measurements with a Comparison of Chemical Evolution Models
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