An end-to-end CNN search for ultra-short-period planets in TESS: from the blend ceiling to the independent validation of TOI-6662 b

We trained a convolutional neural network to detect ultra-short-period planets in TESS photometry, following the procedure now standard in the field: synthetic transits as positives, eclipsing binaries as negatives. Measured that way it reaches an area under the ROC curve of 0.97. Keeping the same m