Fig. 13

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Simulated molecular maps and reconstruction of the predicted classification scores by the S/N and CNN. Left: insertion of a simulated PZ Tel В signal in the real PZ Tel В noise cubes, with same location, Gaussian decay and average S/N = 7.3 as the real data shown as a molecular map in good seeing conditions. Middle-left: insertion of a signal in the PZ Tel B data with location and Gaussian decay of the original signal, but with an average S /N = 1.22 to emulate a signal in bad seeing conditions. Middle-right: S/N probability scores for bad seeing conditions. The planet is not detectable at S/N = 5. Right: CNN probability scores for bad seeing conditions. A very clear conspicuity improvement is observed in probabilistic map, clearly enhancing the planet’s visibility.
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