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

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Table D.1.

2D Scaling relations

Relation	Sample	UL	α	β	δ_intr	P	K	Fig.
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(9)	(10)
M_HI,R25–M_dust	120	1	$0 . 80_{- 0.06}^{+ 0.06}$ $0.80^{+0.06}_{-0.06 }$	$3 . 52_{- 0.04}^{+ 0.04}$ $3.52^{+0.04}_{-0.04 }$	$0 . 37_{- 0.03}^{+ 0.03}$ $0.37^{+0.03}_{-0.03 }$	0.72	0.60	3
M_HI,tot–M_dust	120	1	$0 . 77_{- 0.07}^{+ 0.07}$ $0.77^{+0.07}_{-0.07 }$	$3 . 88_{- 0.04}^{+ 0.04}$ $3.88^{+0.04}_{-0.04 }$	$0 . 43_{- 0.03}^{+ 0.04}$ $0.43^{+0.04}_{-0.03 }$	0.71	0.55	3
M_HI,R25–M_⋆	120	0	$0 . 93_{- 0.05}^{+ 0.05}$ $0.93^{+0.05}_{-0.05 }$	$3 . 63_{- 0.03}^{+ 0.03}$ $3.63^{+0.03}_{-0.03 }$	$0 . 29_{- 0.02}^{+ 0.03}$ $0.29^{+0.03}_{-0.02 }$	0.89	0.65	3
M_H2–M_dust	120	5	$1 . 25_{- 0.06}^{+ 0.06}$ $1.25^{+0.06}_{-0.06 }$	$0 . 08_{- 0.04}^{+ 0.04}$ $0.08^{+0.04}_{-0.04 }$	$0 . 38_{- 0.03}^{+ 0.03}$ $0.38^{+0.03}_{-0.03 }$	0.86	0.66	3
M_gas–M_dust	120	6	$0 . 93_{- 0.04}^{+ 0.04}$ $0.93^{+0.04}_{-0.04 }$	$2 . 87_{- 0.02}^{+ 0.02}$ $2.87^{+0.02}_{-0.02 }$	$0 . 21_{- 0.02}^{+ 0.02}$ $0.21^{+0.02}_{-0.02 }$	0.86	0.70	3
M_gas,tot–M_dust	120	6	$0 . 89_{- 0.05}^{+ 0.05}$ $0.89^{+0.05}_{-0.05 }$	$3 . 25_{- 0.03}^{+ 0.03}$ $3.25^{+0.03}_{-0.03 }$	$0 . 25_{- 0.02}^{+ 0.03}$ $0.25^{+0.03}_{-0.02 }$	0.85	0.66	3
SFR–M_⋆	121	0	$0 . 69_{- 0.07}^{+ 0.07}$ $0.69^{+0.07}_{-0.07 }$	$- 6 . 98_{- 0.05}^{+ 0.05}$ $-6.98^{+0.05}_{-0.05 }$	$0 . 52_{- 0.04}^{+ 0.04}$ $0.52^{+0.04}_{-0.04 }$	0.64	0.38
M_H₂–M_⋆	121	6	$1 . 17_{- 0.07}^{+ 0.07}$ $1.17^{+0.07}_{-0.07 }$	$- 3 . 03_{- 0.04}^{+ 0.05}$ $-3.03^{+0.05}_{-0.04 }$	$0 . 45_{- 0.03}^{+ 0.04}$ $0.45^{+0.04}_{-0.03 }$	0.84	0.56	4
M_H₂–SFR	121	6	$1 . 09_{- 0.08}^{+ 0.08}$ $1.09^{+0.08}_{-0.08 }$	$8 . 74_{- 0.05}^{+ 0.05}$ $8.74^{+0.05}_{-0.05 }$	$0 . 52_{- 0.04}^{+ 0.05}$ $0.52^{+0.05}_{-0.04 }$	0.74	0.61	4
M_H₂–M_dust	121	6	$1 . 26_{- 0.06}^{+ 0.06}$ $1.26^{+0.06}_{-0.06 }$	$0 . 04_{- 0.04}^{+ 0.04}$ $0.04^{+0.04}_{-0.04 }$	$0 . 38_{- 0.03}^{+ 0.04}$ $0.38^{+0.04}_{-0.03 }$	0.86	0.66	4
M_H₂–M_HI,R25	120	0	$0 . 94_{0.10}^{0.10}$ $0.94 ^{ 0.10 }_{ 0.10 }$	$0 . 28_{0.06}^{0.06}$ $0.28 ^{ 0.06 }_{ 0.06 }$	$0 . 68_{0.05}^{0.05}$ $0.68 ^{ 0.05 }_{ 0.05 }$	0.63	0.47	6
M_H₂/HI,R25–M_⋆	120	0	$0 . 60_{0.08}^{0.09}$ $0.60 ^{ 0.09 }_{ 0.08 }$	$- 6 . 35_{0.05}^{0.05}$ $-6.35 ^{ 0.05 }_{ 0.05 }$	$0 . 56_{0.04}^{0.04}$ $0.56 ^{ 0.04 }_{ 0.04 }$	0.51	0.25	6
M_H₂/HI,R25–M_dust/⋆	120	0	$- 0 . 67_{0.22}^{0.22}$ $-0.67 ^{ 0.22 }_{ 0.22 }$	$- 2 . 41_{0.06}^{0.06}$ $-2.41 ^{ 0.06 }_{ 0.06 }$	$0 . 64_{0.04}^{0.05}$ $0.64 ^{ 0.05 }_{ 0.04 }$	-0.26	-0.17	6
M_H₂/M_⋆–sSFR	121	6	$0 . 44_{- 0.07}^{+ 0.07}$ $0.44^{+0.07}_{-0.07 }$	$3 . 15_{- 0.04}^{+ 0.04}$ $3.15^{+0.04}_{-0.04 }$	$0 . 37_{- 0.03}^{+ 0.03}$ $0.37^{+0.03}_{-0.03 }$	0.47	0.37	7
SFE–M_⋆	121	6	$- 0 . 53_{- 0.07}^{+ 0.07}$ $-0.53^{+0.07}_{-0.07 }$	$- 3 . 37_{- 0.04}^{+ 0.04}$ $-3.37^{+0.04}_{-0.04 }$	$0 . 41_{- 0.03}^{+ 0.04}$ $0.41^{+0.04}_{-0.03 }$	-0.57	-0.38	7

SFR_SED–M_H₂	85	0	$0 . 58_{- 0.06}^{+ 0.06}$ $0.58^{+0.06}_{-0.06 }$	$- 5 . 02_{- 0.05}^{+ 0.05}$ $-5.02^{+0.05}_{-0.05 }$	$0 . 41_{- 0.03}^{+ 0.04}$ $0.41^{+0.04}_{-0.03 }$	0.73	0.61	B.1
SFR_FUV+24μm–M_H₂	85	0	$0 . 56_{- 0.05}^{+ 0.05}$ $0.56^{+0.05}_{-0.05 }$	$- 4 . 99_{- 0.04}^{+ 0.04}$ $-4.99^{+0.04}_{-0.04 }$	$0 . 37_{- 0.03}^{+ 0.03}$ $0.37^{+0.03}_{-0.03 }$	0.78	0.64	B.1
SFR_160μm–M_H₂	85	0	$0 . 76_{- 0.04}^{+ 0.04}$ $0.76^{+0.04}_{-0.04 }$	$- 6 . 50_{- 0.03}^{+ 0.03}$ $-6.50^{+0.03}_{-0.03 }$	$0 . 24_{- 0.02}^{+ 0.03}$ $0.24^{+0.03}_{-0.02 }$	0.89	0.77	B.1

Notes. 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 slope α, normalization β, and intrinsic dispersion δ_intr; (7), (8) and (9) Pearson CC and Kendall rank CCs; (10) Reference to figures in the main text (when available). CCs are calculated considering only CO and HI detections.

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