Table 7
Lines used in the A1 analysis to determine abundances for Star 1.
Z | λ | log(gf) | Sourcea | E low | Abundance |
(nm) | [cm-1] | (log (NH) = 12.00) | |||
|
|||||
14 | 568.448 | −1.650 | GARZ | 39955.053 | 6.95 |
14 | 569.043 | −1.870 | GARZ | 39760.285 | 7.10 |
14 | 570.110 | −2.050 | GARZ | 39760.285 | 7.08 |
14 | 577.215 | −1.750 | GARZ | 40991.884 | 7.04 |
14 | 579.307 | −2.060 | GARZ | 39760.285 | 7.15 |
20 | 558.875 | + 0.210 | NBS | 20371.000 | 4.83 |
20 | 559.011 | −0.710 | NBS | 20335.360 | 5.23 |
20 | 559.446 | −0.050 | NBS | 20349.260 | 4.81 |
20 | 560.128 | −0.690 | NBS | 20371.000 | 5.13 |
20 | 615.602 | −2.200 | NBS | 20335.360 | 5.88 |
20 | 645.560 | −1.350 | NBS | 20349.260 | 5.48 |
20 | 817.329 | −0.546 | K88 | 39349.080 | 5.90 |
20 | 820.375 | −0.848 | K88 | 36575.119 | 5.90 |
20 | 829.218 | −0.391 | K88 | 39340.080 | 5.80 |
22 | 546.047 | −2.880 | SK | 386.874 | 4.55 |
22 | 556.271 | −2.870 | MFW | 7255.369 | 4.55 |
22 | 802.484 | −1.140 | MFW | 15156.787 | 4.45 |
22 | 806.825 | −1.280 | MFW | 15108.121 | 4.65 |
22 | 841.229 | −1.483 | MFW | 18482.860 | 4.55 |
22 | 867.527 | −1.669 | MFW | 8602.340 | 4.50 |
22 | 868.299 | −1.941 | MFW | 8492.421 | 4.50 |
22 | 869.233 | −2.295 | MFW | 8436.618 | 4.70 |
22 | 873.471 | −2.384 | MFW | 8492.421 | 4.70 |
26 | 552.554 | −1.330 | FMW | 34121.580 | 6.70 |
26 | 552.890 | −2.020 | FMW | 36079.366 | 7.30 |
26 | 552.916 | −2.730 | FMW | 29371.811 | 7.10 |
26 | 553.275 | −2.150 | FMW | 28819.946 | 6.70 |
26 | 554.394 | −1.140 | FMW | 34017.098 | 6.70 |
26 | 555.798 | −1.280 | FMW | 36079.366 | 6.65 |
26 | 556.021 | −1.190 | FMW | 35767.561 | 6.75 |
26 | 829.351 | −2.126 | K88 | 38678.032 | 6.90 |
26 | 832.705 | −1.525 | FMW | 17726.981 | 6.70 |
Notes. For each line, the atomic number Z, the wavelength λ, the gf value, the lower level excitation potential Elow, and the line abundance are given. The full table is available at the CDS.
References as listed in Kurucz & Bell (1995): http://kurucz.harvard.edu/LINELISTS/LINES/gfall.ref.
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