CON-quest - II. Spatially and spectrally resolved HCN/HCO+ line ratios in local luminous and ultraluminous infrared galaxies

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Volume 686 (June 2024)

A&A, 686 (2024) A48

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Table 5.

Spearman rank coefficients and p-values.

Quantities	ρ	p-value
Global $L_{HCN}^{'} / L_{{HCO}^{+}}^{'}$ $L^\prime_{\rm HCN}/L^\prime_{\rm HCO^+}$ vs.
α_AGN	$- 0 . 17_{- 0.23}^{+ 0.24}$ $-0.17^{+0.24}_{-0.23}$	$0 . 38_{- 0.31}^{+ 0.41}$ $0.38^{+0.41}_{-0.31}$
$log (L_{AGN}^{bol} / {erg s}^{- 1})$ $\log(L_{\mathrm{AGN}}^{\mathrm{bol}}/\mathrm{erg\,s}^{-1})$	$+ 0 . 00_{- 0.26}^{+ 0.27}$ $+0.00^{+0.27}_{-0.26}$	$0 . 44_{- 0.34}^{+ 0.38}$ $0.44^{+0.38}_{-0.34}$
log(L_IR/L_⊙)	$+ 0 . 11_{- 0.26}^{+ 0.25}$ $+0.11^{+0.25}_{-0.26}$	$0 . 42_{- 0.33}^{+ 0.39}$ $0.42^{+0.39}_{-0.33}$
log(SFR/M_⊙ yr⁻¹)	$+ 0 . 09_{- 0.26}^{+ 0.24}$ $+0.09^{+0.24}_{-0.26}$	$0 . 44_{- 0.33}^{+ 0.38}$ $0.44^{+0.38}_{-0.33}$
S₆₀/S₁₀₀	$+ 0 . 02_{- 0.25}^{+ 0.25}$ $+0.02^{+0.25}_{-0.25}$	$0 . 47_{- 0.34}^{+ 0.36}$ $0.47^{+0.36}_{-0.34}$
[N II]₁₂₂/[O III]₈₈	$+ 0 . 50_{- 0.32}^{+ 0.25}$ $+0.50^{+0.25}_{-0.32}$	$0 . 10_{- 0.09}^{+ 0.42}$ $0.10^{+0.42}_{-0.09}$

Resolved $L_{HCN}^{'} / L_{{HCO}^{+}}^{'}$ $L^\prime_{\rm HCN}/L^\prime_{\rm HCO^+}$ vs.
α_AGN	$- 0 . 22_{- 0.22}^{+ 0.23}$ $-0.22^{+0.23}_{-0.22}$	$0 . 31_{- 0.26}^{+ 0.44}$ $0.31^{+0.44}_{-0.26}$
$log (L_{AGN}^{bol} / {erg s}^{- 1})$ $\log(L_{\mathrm{AGN}}^{\mathrm{bol}}/\mathrm{erg\,s}^{-1})$	$+ 0 . 05_{- 0.25}^{+ 0.24}$ $+0.05^{+0.24}_{-0.25}$	$0 . 47_{- 0.34}^{+ 0.36}$ $0.47^{+0.36}_{-0.34}$
log(L_IR/L_⊙)	$+ 0 . 23_{- 0.25}^{+ 0.23}$ $+0.23^{+0.23}_{-0.25}$	$0 . 29_{- 0.25}^{+ 0.45}$ $0.29^{+0.45}_{-0.25}$
log(SFR/M_⊙ yr⁻¹)	$+ 0 . 23_{- 0.25}^{+ 0.22}$ $+0.23^{+0.22}_{-0.25}$	$0 . 29_{- 0.25}^{+ 0.45}$ $0.29^{+0.45}_{-0.25}$
S₆₀/S₁₀₀	$+ 0 . 07_{- 0.24}^{+ 0.24}$ $+0.07^{+0.24}_{-0.24}$	$0 . 47_{- 0.34}^{+ 0.35}$ $0.47^{+0.35}_{-0.34}$
[N II]₁₂₂/[O III]₈₈	$+ 0 . 38_{- 0.32}^{+ 0.26}$ $+0.38^{+0.26}_{-0.32}$	$0 . 21_{- 0.19}^{+ 0.46}$ $0.21^{+0.46}_{-0.19}$

Notes. We performed Spearman rank correlation analyses using the Monte Carlo perturbation plus bootstrapping method as implemented by pymccorrelation (Privon et al. 2020, see Sect. 5.2 for detail). Correlation coefficients ρ and p-values are the median and range of the 16 and 84 percentiles. Corresponding plots are shown in Figs. 2 and 3.

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