An analytic model for [O iii] fine structure emission from high redshift galaxies
ABSTRACT Recent ALMA measurements have revealed bright [O iii] 88 micron line emission from galaxies during the Epoch of Reionization (EoR) at redshifts as large as z ∼ 9. We introduce an analytic model to help interpret these and other upcoming [O iii] 88 micron measurements. Our approach sums over...
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| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2020-12, Vol.499 (3), p.3417-3433 |
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| Hauptverfasser: | , |
| Format: | Artikel |
| Sprache: | eng |
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