Fig. 11
Resulting covariance matrix of the parameters for a given non-photometric night (2010-06-28). The represented parameters are the flux solution C(λ) at every meta-slice wavelength, the atmospheric normalized model parameters , τ and å as well as the grey extinction δT per star. SDSS filters u, g, r and i are also represented (black squares) over the flux solution wavelengths.
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