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Fig. 1

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Positive (lens) and negative (non-lens) examples in our baseline ground-truth data set. The first, second, and third rows show mock lenses with 0.75″ E < 1.30″, 1.30″ < θE < 1.90″, and 1.90″ < θE < 2.50″, respectively. The fourth, fifth, and sixth rows show examples of LRGs, spirals, and random galaxies from the parent sample of galaxies with i-band Kron radius ≥ 0.8″, respectively. This corresponds to the three main classes of negative examples. Cutouts have sizes of 10″ × 10″.

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