Fig. B.2

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Distribution of incorrect classifications (FP and FN) with respect to IE – YE, sSFR, and stellar mass, when selecting quiescent galaxies from the Int catalogues. Also shown is the overall distribution of galaxies in the catalogue (or catalogue subset) on which the selection was performed. Top row: Using the ugriz, Euclid, W1 , W2, and 20 cm photometry from the Int Wide catalogue, excluding only those galaxies with a non-detection in any Euclid band. Centre row: As above, but excluding galaxies without a non-detection in any of the ugriz or Euclid bands. Bottom row: Using the ugriz, Euclid, W1 , W2, and 20 cm photometry from the Int Deep catalogue, excluding only those galaxies with a non-detection in any Euclid band. In each case, we include the values of the F1-score, precision, recall, and @ metrics
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