Table 3
Isotope information for the elements included in the preselected line list.
| Z | El. | I | H | Baryon numbers | Rel. abund. (%) | Reference | Nucl. spin |
|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| 3 | Li | y | n | 6:7 | 7.6:92.4 | Qi et al. (1997) | 1, 1.5 |
| 6 | C | n | n | 12:13 | 99:1 | Chang & Li (1990) | 0.5 |
| 8 | O | 16 | 99.8 | Baertschi (1976); Li et al. (1988) | |||
| 11 | Na | n | 23 | 100 | White et al. (1956) | 1.5 | |
| 12 | Mg | n | n | 24:25:26 | 79:10:11 | Bizzarro et al. (2011) | 2.5 |
| 13 | Al | n | 27 | 100 | White et al. (1956) | 2.5 | |
| 14 | Si | n | n | 28:29:30 | 92:5:3 | Gonfiantini et al. (1997) | 0.5 |
| 16 | S | n | n | 32:33:34 | 95:1:4 | Ding et al. (2001) | 1.5 |
| 20 | Ca | n | 40:42:44 | 97:1:2 | Moore & Machlan (1972) | ||
| 21 | Sc | y | 45 | 100 | Leland (1950) | 3.5 | |
| 22 | Ti | n | n | 46:47:48:49:50 | 8:7:74:5:5 | Shima & Torigoye (1993) | 2.5, 3.5 |
| 23 | V | y | 51 | 99.8 | Flesch et al. (1966) | 3.5 | |
| 24 | Cr | n | n | 50:52:53:54 | 4:84:10:2 | Shields et al. (1966) | 1.5 |
| 25 | Mn | y | 55 | 100 | Leipziger (1963) | 2.5 | |
| 26 | Fe | n | n | 54:56:57 | 6:92:2 | Taylor et al. (1992) | 0.5 |
| 27 | Co | y | 59 | 100 | Leipziger (1963) | 3.5 | |
| 28 | Ni | n | n | 58:60:61:62:64 | 68:26:1:4:1 | Gramlich et al. (1989) | 1.5 |
| 29 | Cu | y | y | 63:65 | 69:31 | Shields et al. (1965) | 1.5, 1.5 |
| 30 | Zn | n | n | 64:66:67:68:70 | 49:28:4:18:1 | Ponzevera et al. (2006) | 2.5 |
| 38 | Sr | n | n | 86:87:88 | 10:7:83 | Moore et al. (1982) | 4.5 |
| 39 | Y | n | 89 | 100 | Collins et al. (1957) | 0.5 | |
| 40 | Zr | n | n | 90:91:92:94:96 | 51:11:17:17:3 | Nomura et al. (1983) | 2.5 |
| 41 | Nb | n | 93 | 100 | White et al. (1956) | 4.5 | |
| 42 | Mo | n | n | 92:94:95:96:97:98:100 | 15:9:16:17:10:24:10 | Mayer & Wieser (2014) | 2.5, 2.5 |
| 44 | Ru | n | n | 96:98:99:100:101:102:104 | 5:2:13:13:17:31:19 | Huang & Masuda (1997) | 2.5, 2.5 |
| 56 | Ba | y | y | 134:135:136:137:138 | 2:7:8:11:72 | Eugster et al. (1969) | 1.5, 1.5 |
| 57 | La | y | 139 | 100 | de Laeter & Bukilic (2005) | 3.5 | |
| 58 | Ce | n | 140:142 | 88:11 | Chang et al. (1995) | ||
| 59 | Pr | y | 141 | 100 | Collins et al. (1957) | 2.5 | |
| 60 | Nd | y | y | 142:143:144:145:146:148:150 | 27:12:24:8:17:6:6 | Zhao et al. (2005) | 3.5, 3.5 |
| 62 | Sm | n | y | 144:147:148:149:150:152:154 | 3:15:11:14:7:27:23 | Chang et al. (2002) | 3.5, 3.5 |
| 63 | Eu | n | y | 151:153 | 48:52 | Chang et al. (1994) | 2.5, 2.5 |
| 64 | Gd | n | n | 154:155:156:157:158:160 | 2:15:20:16:25:22 | Eugster et al. (1970) | 1.5, 1.5 |
| 66 | Dy | n | n | 160:161:162:163:164 | 2:19:25:25:28 | Chang et al. (2001) | 2.5, 2.5 |
Notes. Columns 3 and 4 indicate whether isotopic and/or HFS components are included in the line list (y) or not (n). These fields are empty when the effect does not apply. Column 5 gives the baryon numbers of stable isotopes contributing at least 1% to the abundance in the Solar System. Column 6 gives the corresponding relative isotopic abundances in per cent, with reference in Col. 7. Column 8 gives the nuclear spins of the isotopes with odd baryon numbers (except for Li).
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