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Table 2:

Effective temperature vs. line-ratio calibration table.
Num1 Num2 Stddev Nstars $\lambda_1$ $\lambda_2$ Ele1 Ele2 c0 c1 c2 c3 $T_{\rm eff}^{\rm min}$ $T_{\rm eff}^{\rm max}$ Fit type $^{\dagger}$
... ... ... ... ... ... ... ... ... ... ... ...      
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. $\dagger$ 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); $\lambda_1$ is the wavelength of the first line of the ratio; $\lambda_2$ 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; $T_{\rm eff}^{\rm min}$ and $T_{\rm eff}^{\rm max}$ 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 `` $T{_{\rm eff}}$ vs. r'' - 3, and 4 correspond to the relation `` $T{_{\rm eff}}$ 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 `` $T{_{\rm eff}}$ 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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