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Arrabal Haro , P · 2023

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astro-ph.GA 1

years

2025 1

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CONDITIONAL 1

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Emission-Line Diagnostics at z>4: [OIII]{\lambda}4363/H\gamma

astro-ph.GA · 2025-02-05 · conditional · novelty 4.0

BLAGN at z>4 are distinguished by [NeIII]/[OII], but the full [OIII]/Hgamma versus [NeIII]/[OII] diagram is contaminated by about 40% non-broad-line galaxies, so it cannot robustly separate AGN from star-forming galaxies.

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  • Emission-Line Diagnostics at z>4: [OIII]{\lambda}4363/H\gamma astro-ph.GA · 2025-02-05 · conditional · none · ref 4

    BLAGN at z>4 are distinguished by [NeIII]/[OII], but the full [OIII]/Hgamma versus [NeIII]/[OII] diagram is contaminated by about 40% non-broad-line galaxies, so it cannot robustly separate AGN from star-forming galaxies.