Rapid classification of TESS planet candidates with convolutional neural networks

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Volume 633 (January 2020)

A&A, 633 (2020) A53

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Table 3

TESS objects of interest with a high likelihood of being astrophysical false positives.

TID	TOI	UNK₃	PL₃	EB₃	EB₄	BEB₄
2760710	227.01	0.090	0.000	0.910	0.836	0.024
279740441	273.01	0.574	0.000	0.426	0.000	0.835
425934411	142.01	0.506	0.001	0.493	0.000	0.678
272086159	176.01	0.001	0.000	0.999	0.879	0.003
272086159	176.01	0.002	0.000	0.998	0.800	0.000
237924601	252.01	0.006	0.000	0.994	0.003	0.873
92226327	256.01	0.150	0.000	0.850	0.558	0.276
425934411	142.01	0.157	0.005	0.838	0.000	0.979
425934411	142.01	0.033	0.000	0.966	0.000	0.853
237924601	252.01	0.021	0.107	0.872	0.125	0.592
231702397	122.01	0.199	0.390	0.411	0.057	0.640
307210830	175.02	0.186	0.412	0.401	0.000	0.610
176778112	408.01	0.352	0.014	0.634	0.000	0.520
355703913	111.01 ^(a)	0.055	0.010	0.935	0.005	0.408
237924601	252.01	0.110	0.399	0.491	0.011	0.515

Notes. We only show all classes for the three-class model, and the split EB and BEB classes from the four-class model. ^(a) Marks HATS-34b.

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