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

ABSTRACT We analyse the chemical properties of three z∼ 8 galaxies behind the galaxy cluster SMACS J0723.3-7327, observed as part of the Early Release Observations programme of the James Webb Space Telescope. Exploiting [O iii]λ4363 auroral line detections in NIRSpec spectra, we robustly apply the d...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society Jg. 518; H. 1; S. 425 - 438
Hauptverfasser:	Curti, Mirko, D’Eugenio, Francesco, Carniani, Stefano, Maiolino, Roberto, Sandles, Lester, Witstok, Joris, Baker, William M, Bennett, Jake S, Piotrowska, Joanna M, Tacchella, Sandro, Charlot, Stephane, Nakajima, Kimihiko, Maheson, Gabriel, Mannucci, Filippo, Amiri, Amirnezam, Arribas, Santiago, Belfiore, Francesco, Bonaventura, Nina R, Bunker, Andrew J, Chevallard, Jacopo, Cresci, Giovanni, Curtis-Lake, Emma, Hayden-Pawson, Connor, Jones, Gareth C, Kumari, Nimisha, Laseter, Isaac, Looser, Tobias J, Marconi, Alessandro, Maseda, Michael V, Scholtz, Jan, Smit, Renske, Übler, Hannah, Wallace, Imaan E B
Format:	Journal Article
Sprache:	Englisch
Veröffentlicht:	London Oxford University Press 01.01.2023 Oxford University Press (OUP): Policy P - Oxford Open Option A
Schlagworte:	Astrophysics Chemical properties Cosmology and Extra-Galactic Astrophysics Galactic clusters Galaxies Gas flow Line spectra Metallicity Physics Red shift Space telescopes Star & galaxy formation Star formation Stars & galaxies galaxies: general galaxies: abundances galaxies: evolution galaxies: ISM Galaxies: evolution Galaxies: abundances Galaxies: ISM Galaxies: general
ISSN:	0035-8711, 1365-2966, 1365-2966
Online-Zugang:	Volltext
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Abstract	ABSTRACT We analyse the chemical properties of three z∼ 8 galaxies behind the galaxy cluster SMACS J0723.3-7327, observed as part of the Early Release Observations programme of the James Webb Space Telescope. Exploiting [O iii]λ4363 auroral line detections in NIRSpec spectra, we robustly apply the direct Te method for the very first time at such high redshift, measuring metallicities ranging from extremely metal poor (12 + log(O/H)≈ 7) to about one-third solar. We also discuss the excitation properties of these sources, and compare them with local strong-line metallicity calibrations. We find that none of the considered diagnostics match simultaneously the observed relations between metallicity and strong-line ratios for the three sources, implying that a proper re-assessment of the calibrations may be needed at these redshifts. On the mass–metallicity plane, the two galaxies at z ∼ 7.6 ($\rm log(M_/M_{\odot }) = 8.1, 8.7$) have metallicities that are consistent with the extrapolation of the mass–metallicity relation at z∼2–3, while the least massive galaxy at z ∼ 8.5 ($\rm log(M_/M_{\odot }) = 7.8$) shows instead a significantly lower metallicity. The three galaxies show different level of offset relative to the Fundamental Metallicity Relation, with two of them (at z∼ 7.6) being marginally consistent, while the z∼ 8.5 source deviating significantly, being probably far from the smooth equilibrium between gas flows, star formation, and metal enrichment in place at later epochs.
AbstractList	We analyse the chemical properties of three z∼ 8 galaxies behind the galaxy cluster SMACS J0723.3-7327, observed as part of the Early Release Observations programme of the James Webb Space Telescope. Exploiting [O iii]λ4363 auroral line detections in NIRSpec spectra, we robustly apply the direct Te method for the very first time at such high redshift, measuring metallicities ranging from extremely metal poor (12 + log(O/H)≈ 7) to about one-third solar. We also discuss the excitation properties of these sources, and compare them with local strong-line metallicity calibrations. We find that none of the considered diagnostics match simultaneously the observed relations between metallicity and strong-line ratios for the three sources, implying that a proper re-assessment of the calibrations may be needed at these redshifts. On the mass–metallicity plane, the two galaxies at z ∼ 7.6 ($\rm log(M_/M_{\odot }) = 8.1, 8.7$) have metallicities that are consistent with the extrapolation of the mass–metallicity relation at z∼2–3, while the least massive galaxy at z ∼ 8.5 ($\rm log(M_/M_{\odot }) = 7.8$) shows instead a significantly lower metallicity. The three galaxies show different level of offset relative to the Fundamental Metallicity Relation, with two of them (at z∼ 7.6) being marginally consistent, while the z∼ 8.5 source deviating significantly, being probably far from the smooth equilibrium between gas flows, star formation, and metal enrichment in place at later epochs. ABSTRACT We analyse the chemical properties of three z∼ 8 galaxies behind the galaxy cluster SMACS J0723.3-7327, observed as part of the Early Release Observations programme of the James Webb Space Telescope. Exploiting [O iii]λ4363 auroral line detections in NIRSpec spectra, we robustly apply the direct Te method for the very first time at such high redshift, measuring metallicities ranging from extremely metal poor (12 + log(O/H)≈ 7) to about one-third solar. We also discuss the excitation properties of these sources, and compare them with local strong-line metallicity calibrations. We find that none of the considered diagnostics match simultaneously the observed relations between metallicity and strong-line ratios for the three sources, implying that a proper re-assessment of the calibrations may be needed at these redshifts. On the mass–metallicity plane, the two galaxies at z ∼ 7.6 ($\rm log(M_/M_{\odot }) = 8.1, 8.7$) have metallicities that are consistent with the extrapolation of the mass–metallicity relation at z∼2–3, while the least massive galaxy at z ∼ 8.5 ($\rm log(M_/M_{\odot }) = 7.8$) shows instead a significantly lower metallicity. The three galaxies show different level of offset relative to the Fundamental Metallicity Relation, with two of them (at z∼ 7.6) being marginally consistent, while the z∼ 8.5 source deviating significantly, being probably far from the smooth equilibrium between gas flows, star formation, and metal enrichment in place at later epochs. ABSTRACT We analyse the chemical properties of three z∼ 8 galaxies behind the galaxy cluster SMACS J0723.3-7327, observed as part of the Early Release Observations programme of the James Webb Space Telescope. Exploiting [O iii]λ4363 auroral line detections in NIRSpec spectra, we robustly apply the direct Te method for the very first time at such high redshift, measuring metallicities ranging from extremely metal poor (12 + log(O/H)≈ 7) to about one-third solar. We also discuss the excitation properties of these sources, and compare them with local strong-line metallicity calibrations. We find that none of the considered diagnostics match simultaneously the observed relations between metallicity and strong-line ratios for the three sources, implying that a proper re-assessment of the calibrations may be needed at these redshifts. On the mass–metallicity plane, the two galaxies at z ∼ 7.6 ($\rm log(M_/M_{\odot }) = 8.1, 8.7$) have metallicities that are consistent with the extrapolation of the mass–metallicity relation at z∼2–3, while the least massive galaxy at z ∼ 8.5 ($\rm log(M_/M_{\odot }) = 7.8$) shows instead a significantly lower metallicity. The three galaxies show different level of offset relative to the Fundamental Metallicity Relation, with two of them (at z∼ 7.6) being marginally consistent, while the z∼ 8.5 source deviating significantly, being probably far from the smooth equilibrium between gas flows, star formation, and metal enrichment in place at later epochs. We analyse the chemical properties of three z∼ 8 galaxies behind the galaxy cluster SMACS J0723.3-7327, observed as part of the Early Release Observations programme of the James Webb Space Telescope (JWST). Exploiting [O iii]λ4363 auroral line detections in NIRSpec spectra, we robustly apply the direct Te method for the very first time at such high redshift, measuring metallicities ranging from extremely metal poor (12+log(O/H)≈ 7) to about one-third solar. We also discuss the excitation properties of these sources, and compare them with local strong-line metallicity calibrations. We find that none of the considered diagnostics match simultaneously the observed relations between metallicity and strong-line ratios for the three sources, implying that a proper re-assessment of the calibrations may be needed at these redshifts. On the mass-metallicity plane, the two galaxies at z ∼ 7.6 (⁠log(M∗/M⊙)=8.1,8.7⁠) have metallicities that are consistent with the extrapolation of the mass-metallicity relation at z∼2-3, while the least massive galaxy at z ∼ 8.5 (⁠log(M∗/M⊙)=7.8⁠) shows instead a significantly lower metallicity . The three galaxies show different level of offset relative to the Fundamental Metallicity Relation, with two of them (at z∼ 7.6) being marginally consistent, while the z∼ 8.5 source deviating significantly, being probably far from the smooth equilibrium between gas flows, star formation and metal enrichment in place at later epochs.
Author	Curti, Mirko Scholtz, Jan Maheson, Gabriel Maseda, Michael V Bunker, Andrew J Cresci, Giovanni Kumari, Nimisha Smit, Renske Sandles, Lester Piotrowska, Joanna M Laseter, Isaac D’Eugenio, Francesco Curtis-Lake, Emma Witstok, Joris Baker, William M Arribas, Santiago Looser, Tobias J Amiri, Amirnezam Charlot, Stephane Hayden-Pawson, Connor Übler, Hannah Maiolino, Roberto Jones, Gareth C Mannucci, Filippo Tacchella, Sandro Carniani, Stefano Belfiore, Francesco Wallace, Imaan E B Bennett, Jake S Nakajima, Kimihiko Bonaventura, Nina R Marconi, Alessandro Chevallard, Jacopo
Author_xml	– sequence: 1 givenname: Mirko orcidid: 0000-0002-2678-2560 surname: Curti fullname: Curti, Mirko email: mc2041@cam.ac.uk – sequence: 2 givenname: Francesco orcidid: 0000-0003-2388-8172 surname: D’Eugenio fullname: D’Eugenio, Francesco – sequence: 3 givenname: Stefano orcidid: 0000-0002-6719-380X surname: Carniani fullname: Carniani, Stefano – sequence: 4 givenname: Roberto surname: Maiolino fullname: Maiolino, Roberto – sequence: 5 givenname: Lester surname: Sandles fullname: Sandles, Lester – sequence: 6 givenname: Joris orcidid: 0000-0002-7595-121X surname: Witstok fullname: Witstok, Joris – sequence: 7 givenname: William M orcidid: 0000-0003-0215-1104 surname: Baker fullname: Baker, William M – sequence: 8 givenname: Jake S orcidid: 0000-0002-8573-2993 surname: Bennett fullname: Bennett, Jake S – sequence: 9 givenname: Joanna M orcidid: 0000-0003-1661-2338 surname: Piotrowska fullname: Piotrowska, Joanna M – sequence: 10 givenname: Sandro orcidid: 0000-0002-8224-4505 surname: Tacchella fullname: Tacchella, Sandro – sequence: 11 givenname: Stephane surname: Charlot fullname: Charlot, Stephane – sequence: 12 givenname: Kimihiko orcidid: 0000-0003-2965-5070 surname: Nakajima fullname: Nakajima, Kimihiko – sequence: 13 givenname: Gabriel surname: Maheson fullname: Maheson, Gabriel – sequence: 14 givenname: Filippo orcidid: 0000-0002-4803-2381 surname: Mannucci fullname: Mannucci, Filippo – sequence: 15 givenname: Amirnezam surname: Amiri fullname: Amiri, Amirnezam – sequence: 16 givenname: Santiago surname: Arribas fullname: Arribas, Santiago – sequence: 17 givenname: Francesco orcidid: 0000-0002-2545-5752 surname: Belfiore fullname: Belfiore, Francesco – sequence: 18 givenname: Nina R surname: Bonaventura fullname: Bonaventura, Nina R – sequence: 19 givenname: Andrew J surname: Bunker fullname: Bunker, Andrew J – sequence: 20 givenname: Jacopo orcidid: 0000-0002-7636-0534 surname: Chevallard fullname: Chevallard, Jacopo – sequence: 21 givenname: Giovanni surname: Cresci fullname: Cresci, Giovanni – sequence: 22 givenname: Emma surname: Curtis-Lake fullname: Curtis-Lake, Emma – sequence: 23 givenname: Connor orcidid: 0000-0001-7964-1027 surname: Hayden-Pawson fullname: Hayden-Pawson, Connor – sequence: 24 givenname: Gareth C surname: Jones fullname: Jones, Gareth C – sequence: 25 givenname: Nimisha orcidid: 0000-0002-5320-2568 surname: Kumari fullname: Kumari, Nimisha – sequence: 26 givenname: Isaac surname: Laseter fullname: Laseter, Isaac – sequence: 27 givenname: Tobias J surname: Looser fullname: Looser, Tobias J – sequence: 28 givenname: Alessandro surname: Marconi fullname: Marconi, Alessandro – sequence: 29 givenname: Michael V orcidid: 0000-0003-0695-4414 surname: Maseda fullname: Maseda, Michael V – sequence: 30 givenname: Jan surname: Scholtz fullname: Scholtz, Jan – sequence: 31 givenname: Renske orcidid: 0000-0001-8034-7802 surname: Smit fullname: Smit, Renske – sequence: 32 givenname: Hannah orcidid: 0000-0003-4891-0794 surname: Übler fullname: Übler, Hannah – sequence: 33 givenname: Imaan E B orcidid: 0000-0002-0695-8485 surname: Wallace fullname: Wallace, Imaan E B
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Keywords	galaxies: general galaxies: abundances galaxies: evolution galaxies: ISM Galaxies: evolution Galaxies: abundances Galaxies: ISM Galaxies: general
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Snippet	ABSTRACT We analyse the chemical properties of three z∼ 8 galaxies behind the galaxy cluster SMACS J0723.3-7327, observed as part of the Early Release... We analyse the chemical properties of three z∼ 8 galaxies behind the galaxy cluster SMACS J0723.3-7327, observed as part of the Early Release Observations... ABSTRACT We analyse the chemical properties of three z∼ 8 galaxies behind the galaxy cluster SMACS J0723.3-7327, observed as part of the Early Release... We analyse the chemical properties of three z∼ 8 galaxies behind the galaxy cluster SMACS J0723.3-7327, observed as part of the Early Release Observations...
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SubjectTerms	Astrophysics Chemical properties Cosmology and Extra-Galactic Astrophysics Galactic clusters Galaxies Gas flow Line spectra Metallicity Physics Red shift Space telescopes Star & galaxy formation Star formation Stars & galaxies
Title	The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z ∼ 8
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