Table 8
Lines with cdepth >0.10 not present in observed YJ band.
Wavelength (nm) | Species | Absorptance(a) 1 – F | Synthetic(b) cdepth |
---|---|---|---|
964.20 | Fe I | 0.016 | 0.176 |
969.90 | Ca I | −0.022 | 0.148 |
974.16 | Fe I | 0.018 | 0.107 |
977.10 | Fe I(c) | 0.136 | 0.113 |
982.43 | Ca I | −0.009 | 0.213 |
983.08 | Ca I | 0.005 | 0.102 |
1038.78 | Si I | 0.007 | 0.102 |
1062.08 | Fe I | 0.012 | 0.107 |
1083.49 | Ca I | −0.005 | 0.152 |
1096.03 | Mg I(d) | 0.415 | 0.323 |
1096.03 | Mg I(d) | 0.321 | 0.416 |
1098.75 | Si I(e) | 0.316 | 0.281 |
1166.59 | Fe I | −0.015 | 0.141 |
1181.48 | Ca I | 0.017 | 0.325 |
1182.42 | Ca I | 0.002 | 0.212 |
1187.74 | La II | 0.007 | 0.110 |
1274.37 | Ca I | −0.003 | 0.160 |
1312.07 | Ca I | 0 | 0.106 |
Notes. (a)Observed (1 – F) at wavelength λ0. (b)VALD stellar extraction mode (Teff = 4800 K, log g = 2.67, υmic = 2 km−1, scaled to solar values). (c)The observed absorptance can be explained by Ti I and Si I. (d)Two Mg lines predicted. The observed absorptance can be explained by CN only. (e)The observed absorptance can be explained by CN only.
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