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Table A.1

Gas masses for the DGS, KINGFISH and G11 samples.

MHI [M] MH2 [M]

Name MHI (Ref) Uncertainty (%) HI area (arcmin2) 12 + log(O/H) (Ref) MH2,MW (Ref) M H2, Z μ gal
(1) (2) (3) (4) (5) (6) (7) (8)

DGS
Haro 11 5.01 × 108a,e (1) 50.00 8.36 (1) 2.51 × 108 (1) 1.17 × 109 1.38
Haro 2 3.77 × 108c (2) 16.08 1.6 8.23 (1) 1.26 × 108 (2) 1.03 × 109 1.38
Haro 3 1.13 × 109a (3) 2.13 8.28 (1) 3.02 × 107 (3) 2.01 × 108 1.38
He 2-10 3.10 × 108c (4) 6.45 3.2 8.43 (1) 9.55 × 107 (4) 3.21 × 108 1.39
HS 0017+1055 1.74 × 108a (5) 7.63 (1) 2.15 × 106d (–) 1.18 × 108 1.37
HS 0052+2536 4.82 × 1010a (6) 8.04 (1) 5.94 × 108d (–) 3.26 × 1010 1.38
HS 0822+3542 5.75 × 107b (7) 22.22 0.6 7.32 (1) 9.48 × 105d (–) 5.21 × 107 1.37
HS 1222+3741 7.79 (1) 1.37
HS 1236+3937 7.72 (1) 1.37
HS 1304+3529 7.93 (1) 1.38
HS 1319+3224 7.81 (1) 1.37
HS 1330+3651 7.98 (1) 1.38
HS 1442+4250 3.10 × 108a (5) 2.27 7.60 (1) 3.82 × 106d (–) 2.10 × 108 1.37
HS 2352+2733 2.30 × 1010a (6) 8.40 (1) 1.38
I Zw 18 1.00 × 108c2 (8) 16.08 7.14 (1) 2.71 × 106d (5) 1.49 × 108 1.37
IC 10 4.41 × 107c2 (9) 4.52 8.17 (1) 4.84 × 106 (6) 5.27 × 107 1.38
II Zw 40 5.66 × 108c (10) 16.08 0.3 8.23 (1) 2.83 × 107 (7) 2.41 × 108 1.38
Mrk 1089 1.47 × 1010b (11) 7.91 26.4 8.10 (1) 2.84 × 108 (1) 4.31 × 109 1.38
Mrk 1450 4.30 × 107c (12) 16.08 0.1 7.84 (1) 5.30 × 105d (–) 2.91 × 107 1.37
Mrk 153 6.93 × 108a (13) 7.86 (1) 8.39 × 106d (–) 4.61 × 108 1.37
Mrk 209 2.76 × 107b (13) 6.58 12.2 7.74 (1) 3.09 × 106 (8) 2.50 × 108 1.37
Mrk 930 3.19 × 109c (14) 11.06 0.1 8.03 (1) 3.07 × 107 (1) 6.57 × 108 1.38
NGC 1140 3.50 × 109a (15) 26.71 8.38 (1) 1.91 × 107 (9) 8.02 × 107 1.38
NGC 1569 1.77 × 108b (16) 16.08 24.0 8.02 (1) 7.08 × 105 (10) 1.54 × 107 1.38
NGC 1705 7.67 × 107b (17) 12.50 13.0 8.27 (1) 1.38
NGC 2366 2.93 × 108b (18) 6.76 420.0 7.70 (1) 9.12 × 106d (11) 5.01 × 108 1.37
NGC 4214 3.76 × 108b (16) 16.08 156.0 8.26 (1) 1.62 × 106 (12) 1.16 × 107 1.38
NGC 4449 9.55 × 108b (16) 16.08 144.0 8.20 (1) 2.67 × 107 (13) 2.50 × 108 1.38
NGC 4861 4.12 × 108b (19) 6.27 34.3 7.89 (1) 5.90 × 106d (1) 3.24 × 108 1.37
NGC 5253 1.06 × 108b (20) 5.66 77.0 8.25 (1) 3.02 × 106 (14) 2.26 × 107 1.38
NGC 625 1.10 × 108c (21) 18.18 20.0 8.22 (1) 4.36 × 106 (1) 3.72 × 107 1.38
NGC 6822 1.04 × 108b (22) 10.45 676.0 7.96 (1) 3.58 × 105 (15) 1.05 × 107 1.38
Pox 186 2.00 × 106a,e (23) 7.70 (1) 2.47 × 104d (–) 1.35 × 106 1.37
SBS 0335-052 4.37 × 108b (24) 10.27 0.2 7.25 (1) 5.67 × 106d (16) 3.12 × 108 1.37
SBS 1159+545 6.30 × 107a (5) 7.44 (1) 7.76 × 105d (–) 4.26 × 107 1.37
SBS 1211+540 5.60 × 107c (12) 16.08 0.1 7.58 (1) 6.90 × 105d (–) 3.79 × 107 1.37
SBS 1249+493 1.00 × 109c (25) 48.15 0.06 7.68 (1) 1.23 × 107d (–) 6.77 × 108 1.37
SBS 1415+437 4.37 × 108c (12) 16.08 0.4 7.55 (1) 5.38 × 106d (–) 2.96 × 108 1.37
SBS 1533+574 3.00 × 109c (14) 11.29 0.2 8.05 (1) 3.70 × 107d (–) 2.03 × 109 1.38
Tol 0618-402 8.09 (1) 1.38
Tol 1214-277 3.22 × 108a (5) 7.52 (1) 3.97 × 106d (–) 2.18 × 108 1.37
UGC 4483 2.52 × 107b (26) 5.00 14.4 7.46 (1) 4.06 × 105d (14) 2.23 × 107 1.37
UGC A20 6.92 × 106b (27) 13.82 9.8 7.50 (1) 2.46 × 105d (–) 1.35 × 107 1.37
UM 133 2.15 × 108b (28) 4.38 6.2 7.82 (1) 4.93 × 106d (–) 2.71 × 108 1.37
UM 311 6.09 × 1010b (29) 16.08 21.2 8.36 (1) 9.37 × 107 (1) 4.28 × 108 1.38
UM 448 6.00 × 109a (15) 27.63 8.32 (1) 3.55 × 109 (3) 1.92 × 1010 1.38
UM 461 7.31 × 107b (26) 5.00 2.6 7.73 (1) 1.66 × 106d (3) 9.09 × 107 1.37
VII Zw 403 3.25 × 107b (2) 8.28 10.4 7.66 (1) 6.41 × 105d (17) 3.52 × 107 1.37

KINGFISH
NGC 0337 3.34 × 109 (27) 11.97 8.18 (2) 6.98 × 108 (18) 7.31 × 109 1.38
NGC 0584 1.58 × 108 (27) 35.92 8.43 (2) 4.78 × 108 (18) 1.58 × 109 1.39
NGC 0628 3.72 × 109 (30) 16.08 8.35 (2) 8.71 × 108 (19) 4.17 × 109 1.38
NGC 0855 1.32 × 108 (27) 29.47 8.29 (2) 8.91 × 107 (18) 5.62 × 108 1.38
NGC 0925 4.56 × 109 (30) 16.08 8.25 (2) 6.14 × 108 (19) 4.66 × 109 1.38
NGC 1097 7.56 × 109 (30) 16.08 8.47 (2) 1.67 × 108 (20) 4.59 × 108 1.39
NGC 1266 8.29 (2) 1.33 × 109 (21) 8.39 × 109 1.38
NGC 1291 1.78 × 109 (30) 16.08 8.52 (2) 1.39
NGC 1316 4.73 × 108 (30) 8.77 (2) 1.40
NGC 1377 8.29 (2) 1.38
NGC 1404 8.54 (2) 1.39
IC 0342 9.49 × 109 (31) 16.08 8.46 (3) 1.60 × 109 (20) 4.60 × 109 1.39
NGC 1482 8.01 × 108 (30) 8.11 (2) 3.11 × 109 (19) 4.49 × 1010 1.38
NGC 1512 7.33 × 109 (30) 16.08 8.56 (2) 1.39
NGC 2146 3.89 × 109 (27) 22.10 8.68 (2) 7.77 × 1010 (22) 8.13 × 1010 1.40
Ho II 4.21 × 108 (27) 23.95 7.72 (2) 5.18 × 106d (18) 2.85 × 108 1.37
DDO 053 6.16 × 107 (30) 16.08 7.60 (2) 7.60 × 105d (11) 4.17 × 107 1.37
NGC 2798 2.13 × 109 (30) 16.08 8.34 (2) 3.21 × 109 (19) 1.61 × 1010 1.38
NGC 2841 8.63 × 109 (30) 16.08 8.54 (2) 2.92 × 109 (19) 5.82 × 109 1.39
NGC 2915 3.52 × 108 (30) 16.08 7.94 (2) 4.34 × 106d (–) 2.39 × 108 1.38
Ho I 1.45 × 108 (16) 16.08 7.61 (2) 1.79 × 106d (18) 9.85 × 107 1.37
NGC 2976 1.27 × 108 (30) 16.08 8.36 (2) 5.81 × 107 (19) 2.66 × 108 1.38
NGC 3049 1.21 × 109 (30) 16.08 8.53 (2) 1.80 × 108 (18) 3.75 × 108 1.39
NGC 3077 8.71 × 108 (16) 16.08 8.52 (4) 3.80 × 106 (9) 8.32 × 106 1.39
M 81dwB 1.16 × 107 (16) 16.08 7.84 (2) 1.43 × 105d (18) 7.85 × 106 1.37
NGC 3190 4.27 × 108 (27) 36.84 8.49 (2) 3.93 × 108 (18) 9.87 × 108 1.39
NGC 3184 3.37 × 109 (30) 16.08 8.51 (2) 1.19 × 109 (19) 2.73 × 109 1.39
NGC 3198 6.85 × 109 (27) 26.71 8.34 (2) 1.30 × 109 (18) 6.53 × 109 1.38
IC 2574 1.32 × 109 (30) 16.08 7.85 (2) 3.16 × 106 (19) 1.51 × 108 1.37
NGC 3265 1.75 × 108 (27) 38.68 8.27 (2) 4.39 × 108 (18) 3.04 × 109 1.38
NGC 3351 1.02 × 109 (30) 16.08 8.60 (2) 4.77 × 108 (19) 7.23 × 108 1.39
NGC 3521 8.71 × 109 (30) 16.08 8.39 (2) 4.77 × 109 (19) 1.90 × 1010 1.38
NGC 3621 6.99 × 109 (30) 16.08 8.27 (2) 1.38
NGC 3627 8.46 × 108 (30) 16.08 8.34 (2) 3.21 × 109 (19) 1.61 × 1010 1.38
NGC 3773 9.03 × 107 (30) 16.08 8.43 (2) 4.95 × 107 (18) 1.64 × 108 1.39
NGC 3938 8.00 × 109 (30) 16.08 8.42 (2) 4.38 × 109 (19) 1.52 × 1010 1.38
NGC 4236 2.69 × 109 (30) 16.08 8.17 (2) 9.33 × 107 (18) 1.02 × 109 1.38
NGC 4254 3.76 × 109 (30) 16.08 8.45 (2) 6.82 × 109 (19) 2.06 × 1010 1.39
NGC 4321 2.39 × 109 (30) 16.08 8.50 (2) 5.34 × 109 (19) 1.28 × 1010 1.39
NGC 4536 1.73 × 109 (30) 16.08 8.21 (2) 1.72 × 109 (19) 1.57 × 1010 1.38
NGC 4559 4.09 × 109 (30) 16.08 8.29 (2) 1.92 × 108 (18) 1.21 × 109 1.38
NGC 4569 1.55 × 108 (30) 16.08 8.58 (2) 1.14 × 109 (19) 1.90 × 109 1.39
NGC 4579 5.47 × 108 (30) 16.08 8.54 (2) 1.89 × 109 (19) 3.77 × 109 1.39
NGC 4594 2.60 × 108 (30) 16.08 8.54 (2) 2.16 × 108 (19) 4.31 × 108 1.39
NGC 4625 1.00 × 109 (30) 16.08 8.35 (2) 2.09 × 107 (18) 1.00 × 108 1.38
NGC 4631 8.77 × 109 (30) 16.08 8.12 (2) 1.10 × 109 (19) 1.52 × 1010 1.38
NGC 4725 3.59 × 109 (30) 16.08 8.35 (2) 2.16 × 109 (19) 1.03 × 1010 1.38
NGC 4736 4.03 × 108 (30) 16.08 8.31 (2) 4.41 × 108 (19) 2.54 × 109 1.38
DDO 154 3.55 × 108 (16) 16.08 7.54 (2) 4.37 × 106d (23) 2.40 × 108 1.37
NGC 4826 2.77 × 108 (30) 16.08 8.54 (2) 4.80 × 108 (19) 9.58 × 108 1.39
DDO 165 1.12 × 108 (27) 14.74 7.63 (2) 1.38 × 106d (18) 7.60 × 107 1.37
NGC 5055 5.59 × 109 (30) 16.08 8.40 (2) 2.73 × 109 (19) 1.04 × 1010 1.38
NGC 5398 2.48 × 108 (27) 11.97 8.35 (2) 1.38
NGC 5408 3.22 × 108 (30) 16.08 7.81 (2) 3.97 × 106d (–) 2.18 × 108 1.37
NGC 5457 1.16 × 1010 (16) 16.08 8.42 (5) 1.38
NGC 5474 9.71 × 108 (27) 24.87 8.31 (2) 5.88 × 107 (18) 3.38 × 108 1.38
NGC 5713 5.51 × 109 (30) 16.08 8.24 (2) 3.39 × 109 (19) 2.69 × 1010 1.38
NGC 5866 2.85 × 108 (30) 8.47 (2) 6.38 × 108 (19) 1.76 × 109 1.39
NGC 6946 3.58 × 109 (30) 16.08 8.40 (2) 4.50 × 109 (19) 1.71 × 1010 1.38
NGC 7331 8.85 × 109 (30) 16.08 8.34 (2) 6.70 × 109 (19) 3.36 × 1010 1.38
NGC 7793 8.75 × 108 (30) 16.08 8.31 (2) 1.38

G11
M 83 5.13 × 109 (31) 5.00 8.62 (6) 8.65 × 108 (20) 1.19 × 109 1.39
NGC 1808 1.78 × 109 (31) 9.46 9.10 (7) 1.75 × 109 (20) 2.64 × 108 1.44
NGC 7552 4.79 × 109 (31) 16.08 8.35 (8) 1.38
M 82 8.91 × 108 (31) 10.29 8.51 (8) 4.43 × 108 (20) 1.01 × 109 1.39
NGC 1068 2.24 × 109 (31) 18.35 9.00 (7) 7.26 × 109 (20) 1.74 × 109 1.43
NGC 0891 7.59 × 109 (31) 16.08 8.90 (7) 5.75 × 109 (20) 2.19 × 109 1.42
MCG +02-04-025 1.74 × 109 (31) 16.08 8.52 (9) 1.39
NGC 7469 1.51 × 109 (31) 16.08 8.70 (10) 6.28 × 109 (20) 6.00 × 109 1.40
NGC 5256 8.53 (9) 9.92 × 109 (20) 2.07 × 1010 1.39
NGC 5953 5.75 × 108 (31) 16.08 8.73 (7) 1.62 × 109 (20) 1.34 × 109 1.40
M 51 5.01 × 109 (31) 5.63 8.55 (8) 3.95 × 109 (20) 7.53 × 109 1.39
NGC 3995 6.17 × 109 (31) 16.08 8.66 (7) 1.40
NGC 3994 2.82 × 109 (31) 16.08 8.61 (7) 1.39
NGC 6052 3.80 × 109 (31) 16.08 8.65 (7) 3.00 × 109 (20) 3.61 × 109 1.40
NGC 1222 1.20 × 109 (31) 16.08 8.57 (7) 7.23 × 108 (21) 1.26 × 109 1.39
NGC 7674 1.07 × 1010 (31) 16.08 8.14 (9) 6.34 × 109 (20) 7.99 × 1010 1.38
NGC 4670 1.66 × 108 (31) 16.08 8.30 (7) 9.00 × 106 (20) 5.42 × 107 1.38

Notes. (1) Galaxy name. (2) Final HI mass in solar masses (the HI masses for the DGS have been corrected to match the extent of the dust aperture). . (3) Uncertainty on the HI mass in %. (4) HI area used to correct the DGS HI masses, in arcmin2, assuming a Gaussian mass distribution profile. (5) Metallicity in term of 12 + log(O/H). (6) Final H2 mass derived with XCO,MW in solar masses. (7) Final H2 mass derived with XCO,Z, going as: XCO,Z∝    Z-2, in solar masses. (8) Mean atomic weight of the galaxy, computed as μgal = 1/(1 − Y − Zgal). The total gas mass can be obtained using Eq. (3) (i.e., Col. 8 × (Col. 2 + Cols. 6 or 7)).

(a)

For these galaxies, no information was available on the extent of the Hi observations. The quoted Hi mass is thus the total Hi mass (diamonds in Fig. 4).

(b)

For these galaxies, we were able to correct the Hi mass and to rescale it to the Hi mass contained in the IR aperture (triangles in Fig. 4).

(c)

For these galaxies, the Hi extent is similar to the IR aperture size and we consider that the total Hi mass corresponds to the Hi mass within the IR aperture (crosses in Fig. 4)

(c2)

For these galaxies, the Hi mass corresponding to the dust emitting region is given in the reference, and is the mass quoted here.

(d)

For these galaxies, the H2 mass correction was applied : i.e. non-detections or absence of data were replaced by 0.012 ×MHI for MH2,MW and 0.68 ×MHI for MH2,Z for galaxies with 12 + log(O/H) 8.1.

(e)

For these 2 galaxies, the Hii mass has a significant contribution to the total gas mass : MHII~ 1.2 ×MHI for Haro 11 from Cormier et al. (2012) and MHII~MHI for Pox186 from Gil de Paz et al. (2003) in the XCO,MW case, and has to be taken into account to estimate the total gas mass.

Reference. References for metallicities: (1) Madden et al. (2013); (2) Kennicutt et al. (2011); (3) McCall et al. (1985); (4) McQuade et al. (1995); (5) Kennicutt et al. (2003); (6) Pilyugin et al. (2006); (7) Galametz et al. (2011); (8) Moustakas et al. (2010); (9) Veilleux et al. (1995); (10) Bonatto & Pastoriza (1990).References for HI masses: (1) Cormier et al. (2014); (2) Thuan et al. (2004); (3) Gordon & Gottesman (1981); (4) Sauvage et al. (1997); (5) Pustilnik & Martin (2007); (6) MacHattie et al. (in prep.); (7) Chengalur et al. (2006); (8) Lelli et al. (2012); (9) Huchtmeier & Richter (1988); (10) Bettoni et al. (2003); (11) Williams et al. (1991); (12) Huchtmeier et al. (2005); (13) Thuan & Martin (1981); (14) Thuan et al. (1999); (15) Davoust & Contini (2004); (16) Walter et al. (2008); (17) Meurer et al. (1998); (18) Hunter et al. (2011); (19) van Eymeren et al. (2009); (20) López-Sánchez et al. (2012); (21) Cannon et al. (2004); (22) de Blok & Walter (2006); (23) Begum & Chengalur (2005); (24) Ekta et al. (2009); (25) Pustilnik et al. (2002); (26) van Zee et al. (1998); (27) Paturel et al. (2003); (28) Ekta & Chengalur (2010); (29) Moles et al. (1994); (30) Draine et al. (2007); (31) Galametz et al. (2011).References for H2 masses: (1) Cormier et al. (2014); (2) Israel (2005); (3) Sage et al. (1992); (4) Kobulnicky et al. (1995); (5) Leroy et al. (2007); (6) Leroy et al. (2006); (7) Bettoni et al. (2003); (8) Young et al. (1995); (9) Albrecht et al. (2004); (10) Greve et al. (1996); (11) Schruba et al. (2012); (12) Walter et al. (2001); (13) Böttner et al. (2003); (14) Taylor et al. (1998); (15) Gratier et al. (2010); (16) Dale et al. (2001b); (17) Leroy et al. (2005); (18) Wilson et al. (2012); (19) Draine et al. (2007); (20) Galametz et al. (2011); (21) Young et al. (2011); (22) Young & Knezek (1989); (23) Leroy et al. (2009).Note on mass references: The references given here are where the original measurement was found. If a correction was applied, the quoted masses are the corrected masses (see ) and not the original masses. If no correction was applied, the quoted masses are the original masses. Note that some galaxies have a molecular gas mass but no reference : this means that the molecular gas mass has been corrected (see d) but that no measurements of the molecular gas mass is available in the literature.

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