Table A.1
Breakdown of basic properties of the galaxy sample by category.
| Galaxy | Hubble | B | SFR | M HI | M H2 | LK | R | V | References |
| type T | μG | M⊙ yr-1 | 108M⊙ | 108M⊙ | 108 erg s-1 | kpc | km s-1 | for columns | |
| 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 3–7, 9 |
|
|
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| Dwarf and Magellanic-type | |||||||||
|
|
|||||||||
| NGC 292 (SMC) | 8.9 | 3.2 | 0.05 | 4.2 | 0.3 | 6.8 | 2.9 | 43 | 1, 1, 1, 40, 50, 16 |
| NGC 1569 | 9.6 | 14.0 | 0.25 | 0.6 | 0.4 | 14 | 1.8 | 39 | 1, 12, 23, 58, 24, 24 |
| NGC 2976 | 5.2 | 5.7 | 0.09 | 2.0 | 0.6 | 26 | 3.1 | 58 | 1, 13, 13, 13, 24, 24 |
| NGC 3239 | 9.8 | 6.9 | 0.25 | 13 | N/A | 8.2 | 6.0 | 95 | 1, 1, 1, –, 24, 24 |
| NGC 4027 | 7.8 | 9.0 | 1.82 | 40 | 4.7 | 439 | 10 | 98 | 1, 1, 1, 41, 24, 24 |
| NGC 4214 | 9.8 | 13.0 | 0.11 | 5.0 | 0.1 | 10 | 3.6 | 42 | 54, 13, 13, 13, 24, 13 |
| NGC 4236 | 8.0 | 4.4 | 0.11 | 15 | 0.9 | 9.4 | 14 | 87 | 1, 1, 1, 55, 24, 51 |
| NGC 4449 | 9.8 | 12.0 | 0.37 | 16 | 0.1 | 46 | 3.8 | 59 | 1, 13, 13, 13, 49, 24 |
| NGC 4605 | 5.0 | 6.4 | 0.17 | 2.0 | 0.4 | 48 | 4.6 | 61 | 1, 1, 1, 56, 24, 24 |
| NGC 4618 | 8.6 | 6.0 | 0.18 | 11 | N/A | 37 | 4.8 | 66 | 1, 1, 1, –, 24, 24 |
| NGC 4656 | 9.0 | 4.7 | 0.85 | 50 | N/A | 7.2 | 18 | 60 | 1, 1, 1, –, 24, 24 |
| NGC 5204 | 8.9 | 6.3 | 0.05 | 6.3 | N/A | 5.8 | 3.4 | 55 | 1, 1, 1, –, 24, 24 |
| NGC 6822 | 9.8 | 4.0 | 0.02 | 1.4 | 0.2 | 1.1 | 1.1 | 92 | 1, 1, 1, 42, 49, 26 |
| UGC 11861 | 7.6 | 5.4 | 0.48 | 87 | N/A | 183 | 10 | 114 | 1, 1, 1, –, 24, 24 |
| UGC 5456 | 9.3 | 3.4 | 0.02 | 1.9 | N/A | 5.7 | 2.5 | 26 | 10, 14, 24, –, 24, 24 |
| HoII | 9.9 | 6.6 | 0.05 | 7.9 | 0.4 | 8.4 | 3.9 | 29 | 4, 13, 13, 13, 24, 13 |
| IC 10 | 9.9 | 13.5 | 0.06 | 0.9 | 0.6 | 3.8 | 0.7 | 52 | 5, 15, 1, 42, 49, 16 |
| IC 1613 | 9.9 | 2.8 | <0.01 | 0.6 | 0.1 | 0.2 | 1.7 | 26 | 1, 1, 1, 42, 50, 16 |
| IC 2574 | 8.9 | 4.0 | 0.07 | 19 | 0.8 | 1.8 | 7.7 | 46 | 1, 13, 13, 13, 50, 24 |
| LMC | 9.1 | 4.3 | 0.26 | 5.0 | 1.4 | 31 | 4.7 | 46 | 1, 1, 1, 43, 50, 16 |
|
|
|||||||||
| Spiral | |||||||||
|
|
|||||||||
| NGC 224 (M 31) | 3.0 | 7.0 | 0.60 | 39 | 2.7 | 421 | 19 | 256 | 11, 16, 25, 57, 49, 16 |
| NGC 598 (M 33) | 5.9 | 6.1 | 0.24 | 14 | 3.3 | 35 | 8.7 | 100 | 11, 15, 26, 26, 49, 16 |
| NGC 628 | 5.2 | 6.0 | 0.81 | 50 | 10 | 213 | 11 | 217 | 4, 13, 13, 13, 49, 13 |
| NGC 891 | 3.1 | 13.0 | 3.48 | 80 | 35 | 647 | 16 | 212 | 11, 17, 27, 23, 49, 16 |
| NGC 925 | 7.0 | 6.0 | 0.56 | 63 | 2.5 | 110 | 14 | 104 | 4, 13, 13, 13, 24, 13 |
| NGC 1097 | 3.3 | 13.0 | 5.90 | 83 | 94 | 1390 | 19 | 219 | 11, 12, 28, 44, 49, 16 |
| NGC 1365 | 3.2 | 9.0 | 7.00 | 130 | 170 | 2229 | 31 | 198 | 11, 16, 30, 30, 49, 16 |
| NGC 1566 | 4.0 | 13.0 | 3.53 | 74 | 13 | 140 | 7.4 | 123 | 11, 12, 31, 52, 24, 31 |
| NGC 2403 | 6.0 | 5.7 | 0.38 | 32 | 0.2 | 74 | 10 | 120 | 4, 13, 13, 13, 49, 13 |
| NGC 2841 | 2.9 | 7.2 | 0.74 | 126 | 3.2 | 1633 | 16 | 319 | 4, 13, 13, 13, 49, 13 |
| NGC 2903 | 4.0 | 7.9 | 3.00 | 44 | 22 | 662 | 16 | 188 | 4, 8, 8, 8, 49, 24 |
| NGC 3031 (M 81) | 2.4 | 7.5 | 0.76 | 27 | 2.2 | 844 | 14 | 216 | 11, 18, 32, 23, 49, 24 |
| NGC 3184 | 5.9 | 7.2 | 0.90 | 40 | 16 | 261 | 11 | 208 | 4, 13, 13, 13, 24, 13 |
| NGC 3198 | 5.2 | 4.9 | 0.93 | 126 | 6.3 | 303 | 17 | 137 | 4, 13, 13, 13, 24, 13 |
| NGC 3627 | 3.1 | 10.4 | 2.22 | 10 | 13 | 838 | 12 | 174 | 4, 13, 13, 13, 49, 13 |
| NGC 3628 | 3.1 | 9.0 | 2.15 | 34 | 37 | 365 | 14 | 215 | 9, 12, 36, 23, 49, 16 |
| NGC 3992 (M 109) | 4.0 | 6.0 | 1.40 | 80 | N/A | 2319 | 27 | 295 | 11, 21, 24, –, 49, 24 |
| NGC 4254 (M 99) | 5.2 | 16.0 | 5.34 | 17 | 85 | 993 | 13 | 299 | 11, 12, 23, 23, 24, 24 |
| NGC 4414 | 5.2 | 15.0 | 4.20 | 41 | 24 | 1297 | 10 | 217 | 11, 19, 24, –, 24, 19 |
| NGC 4594 (M 104) | 1.1 | 6.0 | 0.19 | 13 | 0.1 | 1831 | 11 | 232 | 11, 12, 37, 55, 49, 29 |
| NGC 4736 (M 94) | 2.3 | 11.7 | 0.48 | 5.0 | 3.9 | 428 | 3.3 | 181 | 4, 13, 13, 13, 49, 16 |
| NGC 4826 (M 64) | 2.2 | 5.9 | 0.28 | 5.5 | 18 | 494 | 8.1 | 152 | 8, 12, 8, 8, 49, 24 |
| NGC 5055 | 4.0 | 8.5 | 2.12 | 126 | 50 | 1257 | 18 | 218 | 4, 13, 13, 13, 49, 13 |
| NGC 5194 (M 51) | 4.0 | 13.0 | 3.13 | 32 | 25 | 881 | 13 | 219 | 4, 13, 13, 13, 49, 13 |
| NGC 5236 (M 83) | 5.0 | 12.0 | 2.34 | 90 | 32 | 710 | 8.9 | 170 | 7, 12, 13, 23, 49, 22 |
| NGC 5457 (M 101) | 5.9 | 6.4 | 0.57 | 142 | 38 | 747 | 25 | 274 | 3, 3, 38, 45, 49, 38 |
| NGC 5775 | 5.1 | 11.0 | 3.60 | 16 | 75 | 1224 | 16 | 187 | 11, 20, 23, 23, 24, 24 |
| NGC 5907 | 5.2 | 5.0 | 2.17 | 69 | 9.0 | 1160 | 30 | 226 | 11, 17, 35, 35, 49, 16 |
| NGC 6946 | 5.9 | 12.7 | 3.24 | 63 | 40 | 540 | 9.9 | 314 | 4, 13, 13, 13, 49, 16 |
| NGC 7331 | 3.9 | 9.4 | 2.99 | 126 | 50 | 1825 | 22 | 252 | 4, 13, 13, 13, 49, 13 |
| IC 342 | 6.0 | 9.0 | 1.89 | 16 | 75 | 352 | 10 | 230 | 11, 12, 39, 23, 49, 16 |
|
|
|||||||||
| Massive starburst/LIRG | |||||||||
|
|
|||||||||
| NGC 253 | 5.1 | 15.0 | 4.94 | 19 | 70 | 1051 | 15 | 189 | 11, 16, 28, 23, 49, 16 |
| NGC 3034 (M 82) | 7.2 | 35.0 | 7.87 | 7.5 | 20 | 451 | 6.3 | 200 | 2, 12, 32, 47, 49, 53 |
| NGC 3256 | 4.0 | 25.0 | 80.7 | 62 | 710 | 3793 | 30 | 123 | 6, 6, 33, 48, 24, 33 |
| ARP 220 | 9.3 | 27.0 | 150 | 46 | 275 | 1407 | 17 | 175 | 6, 6, 34, 46, 24, 24 |
Notes. Data for Col. 2, and 8 are from HyperLeda and NED.
Reference. (1) Jurusik et al. (2014); (2) Adebahr et al. (2013); (3) Berkhuijsen 2016; (4) Braun et al. 2007; (5) Chyży et al. 2016; (6) Drzazga et al. 2011; (7) Neininger et al. 1993; (8) Heesen et al. 2014; (9) Nikiel-Wroczyński et al. 2013; (10) this paper; (11) Van Eck et al. 2015; (12) Calzetti et al. 2010; (13) Leroy et al. 2008; (14) Roychowdhury et al. 2012; (15) Woo et al 2008; (16) Tabatabaei et al. 2016; (17) Misiriotis et al. 2001; (18) Karachentsev et al. 2007; (19) de Blok et al. 2014; (20) Irvin 1994; (21) Martinet & Friedli 1997; (22) Heald et al. 2016; (23) Liu et al. 2015; (24) LEDA; (25) Cram et al. 1980; (26) Gratier et al. 2010; (27) Sancisi & Allen 1979; (28) Koribalski et al. 2004; (29) van der Marel et al. 1994; (30) Lindblad 1999; (31) Pence et al. 1990; (32) Chynoweth et al. 2008; (33) English et al. 2003; (34) Baan et al. 1987; (35) Dumke et al. 1997; (36) Huchtmeier et al. 1985; (37) Bajaja et al. 1984; (38) Walter et al. 2008; (39) Rots 1979; (40) Leroy et al. 2007; (41) Casasola et al. 2004; (42) Mateo 1998; (43) Cohen et al. 1988; (44) Crosthwaite 2002; (45) Kenney et al. 1991; (46) Papadopoulos et al. 2012; (47) Young & Scoville 1984; (48) Sargent et al. 1989; (49) Jarrett et al. 2003; (50) NED; (51) Chyży et al. 2011; (52) Combes et al. 2014; (53) Sofue et al. 1999; (54) Kepley et al. 2011; (55) Wilson et al. 2012; (56) Throson & Bally 1987; (57) Dame et al. 1993; (58) Israel 1988.
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