Impact of observational errors in the predicted absolute flux values of theoretical atmospheric models for the solar atmospheric parameters. We generate a distribution of absolute continuum flux based on 104 MC simulations assuming Gaussian uncertainties of 50 K, 0.1 dex, and 0.07 dex for Teff, log g, and [Fe/H], respectivelly. The typical standard deviation found in this distribution is ≈1.3 × 105 erg cm-2 s-1.
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