Amaryllis: A digital twin of the earliest galaxies in the Universe

Open Access

Table 2.

Correlations of [OIII]/[CII] in Amaryllis.

	log U_ion	$log \frac{{SFR}_{3 Myr}}{{SFR}_{50 Myr}}$ $\log \frac{\mathrm{SFR}_{3\,\mathrm{Myr}}}{\mathrm{SFR}_{50\,\mathrm{Myr}}}$	$log \frac{n}{{cm}^{- 3}}$ $\log \frac{\mathrm{n}}{\mathrm{cm}^{-3}}$	$log \frac{Z}{Z_{⊙}}$ $\log \tfrac{Z}{Z_{\odot}}$
r_s	0.64	0.39	−0.11	0.26
p	1.4 × 10⁻⁵	1.5 × 10⁻²	5 × 10⁻¹	1.1 × 10⁻²

Notes. Spearman correlation coefficients (r_s) and p-values for the relation between [OIII]/[CII] and the selected physical properties.

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