Exploring the interplay of dust and gas phases in DustPedia star-forming galaxies

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Table D.2.

3D Scaling relations

Relation	Sample	UL	α	β	γ	δ_intr	Fig.
(1)	(2)	(3)	(4)	(5)	(6)	(7)
x: M_⋆, y: SFR, z:M_H₂	115	0	$0 . 79_{- 0.07}^{+ 0.07}$ $0.79^{+0.07}_{-0.07}$	$0 . 51_{- 0.07}^{+ 0.07}$ $0.51^{+0.07}_{-0.07}$	$0 . 86_{- 0.03}^{+ 0.03}$ $0.86^{+0.03}_{-0.03}$	$0 . 24_{- 0.05}^{+ 0.05}$ $0.24^{+0.05}_{-0.05}$	Fig. 5
x: M_dust, y: M_{HI, R25}, z:M_H₂	115	0	$1 . 38_{- 0.10}^{+ 0.10}$ $1.38^{+0.10}_{-0.10}$	$- 0 . 24_{- 0.10}^{+ 0.10}$ $-0.24^{+0.10}_{-0.10}$	$1 . 38_{- 0.53}^{+ 0.54}$ $1.38^{+0.54}_{-0.53}$	$0 . 34_{- 0.03}^{+ 0.03}$ $0.34^{+0.03}_{-0.03}$	Fig. 5

Notes. Three-dimensional scaling relations: best-fit parameters and correlation coefficients. Columns: (1) Scaling relation; (2) Total number of objects with available atomic and/or molecular gas measurements; (3) Number of detection of the corresponding gas measurements; (4), (5) and (6) Best-fit parameters, namely slopes α and β, normalization γ, and intrinsic dispersion δ_intr; (7) Reference to figure.

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