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Table 3:

Extreme-UV flux excess factors w as a function of the effective temperature and $\gamma $, needed to explain the $\Delta T_{\rm eff}^f$ underestimations affecting the $T_{\rm eff}^f$ values for supergiants.
    $w(\gamma)$
$T_{\rm eff}$ $\Delta T_{\rm eff}^f$ $\gamma =1.0$ $\gamma = 1.5$ $\gamma = 2.0$
K K      
10 000 -500 10.73 9.96 9.19
  -1000 21.94 21.02 20.09
  -1500 34.80 33.69 32.59
  -2000 49.45 48.14 46.83
15 000 -500 1.78 1.36 0.92
  -1000 2.68 2.18 1.68
  -1500 3.64 3.08 2.52
  -2000 4.70 4.06 3.43
20 000 -500 1.32 1.05 0.79
  -1000 1.67 1.37 1.08
  -1500 2.04 1.71 1.39
  -2000 2.43 2.08 1.72
25 000 -500 1.20 1.06 0.92
  -1000 1.41 1.27 1.11
  -1500 1.64 1.48 1.32
  -2000 1.89 1.71 1.53
30 000 -500 1.14 1.04 0.95
  -1000 1.28 1.18 1.08
  -1500 1.43 1.32 1.22
  -2000 1.59 1.47 1.36

The estimates are done for $\log g = 3.0$.


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