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Fig. 12.

image

Error in the estimation P − P0 (Jy), as a function of binned input S0 (Jy), for the set of 10 000 simulated QUIJOTE sky patches with |b|≤10° (left) and the set of 10 000 simulated QUIJOTE sky patches with |b|> 10° (right) at 11 GHz. Bayesian estimations for a perfect photometry of the source total flux density S0 appear in blue, whereas Bayesian estimations including a 0.3 Jy uncertainty in S0 are shown in orange. Error bars show the 68.27% interval of the distribution of results in each case. Filled circles indicate the median of the distribution, and dots indicate the average value of the distribution. Orange points and lines have been slightly displaced to the right in order to make the figure more readable.

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