Spatially resolved star-formation relations of dense molecular gas in NGC 1068

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Table 3.

Spearman rank parameters for different scaling relations.

	SFE_dense vs. Σ_star	F_dense vs. Σ_star	SFE_dense vs. σ_HCN	F_dense vs. σ_HCN	Σ_SFR vs. F_dense	T_dep vs. b_HCN	SFE_dense vs. F_dense
56 pc	0.10	–	−0.22	–	–	−0.19	–
100 pc	0.15	0.40	−0.28	0.10	0.22	–0.43	0.03
400 pc	0.59	0.67	−0.06	0.50	0.62	–0.66	0.34

Notes. We list the Spearman rank parameters (ρ_sp) for the different scaling relations and spatial scales studied in Sect. 6. As in Table 1, values highlighted in boldface identify correlations that are statistically significant; these are characterised by p-values < 1% and |ρ_sp|> 0.4.

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