Num1 | Num2 | Stddev | Nstars | ![]() |
![]() |
Ele1 | Ele2 | c0 | c1 | c2 | c3 |
![]() |
![]() |
Fit type
![]() |
... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | |||
92 | 189 | 92 | 406 | 6237.33 | 6274.66 | SiI | VI | 5052.06 | 754.45 | 169.26 | -91.20 | 4556 | 6287 | 6 |
93 | 190 | 85 | 415 | 6237.33 | 6285.17 | SiI | VI | 5089.04 | 811.62 | 191.03 | -113.42 | 4578 | 6361 | 6 |
94 | 196 | 118 | 421 | 6237.33 | 6240.65 | SiI | FeI | 4342.15 | 1056.95 | 0.00 | 0.00 | 4578 | 6374 | 1 |
95 | 200 | 97 | 433 | 6243.82 | 6258.11 | SiI | TiI | 4564.66 | 1335.20 | 0.00 | 0.00 | 4556 | 6403 | 1 |
96 | 201 | 77 | 434 | 6243.82 | 6261.10 | SiI | TiI | 4486.31 | 1488.62 | 13.19 | -142.17 | 4556 | 6403 | 2 |
97 | 202 | 83 | 423 | 6243.82 | 6216.35 | SiI | VI | 5596.97 | 1546.76 | 309.90 | -342.97 | 4556 | 6289 | 6 |
98 | 203 | 72 | 381 | 6243.82 | 6224.51 | SiI | VI | 5105.05 | 729.82 | 0.00 | 0.00 | 4556 | 6136 | 5 |
99 | 204 | 73 | 425 | 6243.82 | 6251.83 | SiI | VI | 5346.56 | 890.69 | 0.00 | 0.00 | 4556 | 6276 | 5 |
100 | 205 | 80 | 404 | 6243.82 | 6274.66 | SiI | VI | 5179.51 | 809.52 | 0.00 | 0.00 | 4556 | 6287 | 5 |
101 | 206 | 81 | 424 | 6243.82 | 6285.17 | SiI | VI | 5230.92 | 856.44 | 0.00 | 0.00 | 4556 | 6361 | 5 |
102 | 211 | 107 | 434 | 6243.82 | 6240.65 | SiI | FeI | 4338.27 | 1448.16 | 0.00 | 0.00 | 4556 | 6403 | 1 |
... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | ... |
Notes.
The columns correspond to the following: num1 is the final ID number of the line ratio; num2 is the initial ID number of the line ratio; stddev is the final standard deviation for each calibration; nstars is the number of stars used for the calibration of each line ratio (out of a total of 451);
is the wavelength of the first line of the ratio;
is the wavelength of the second line of the ratio; ele1 is the chemical element of the first line of the ratio; ele2 is the element of the second line of the ratio; c0, c1, c2 and c3 are the fitting coefficients for each line-ratio calibration;
and
are the limits in effective temperature of the stars used to calibrate each line ratio; fit type is the type of function used for the calibration used: the numbers 1, and 2 correspond to the relation ``
vs. r'' - 3, and 4 correspond to the relation ``
vs. 1/r''
but the spectral lines are inverted in this table for ease of use, and
the numbers 5 and 6 correspond to the relations ``
vs. log(r)''.
The numbers 2, 4, and 6 correspond to 3rd order
polynomial functions and the numbers 1, 3, 5 correspond to
straight line functions. This is easily noticed in the coefficients c2 and c3 (set to zero in straight line fits).
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