Chapter 10 of 15
False positives
Many transit-like dips are not planets on the target star. A dip is evidence; vetting asks what else could make it. This is where SetuHQ's own checks live.
How often, and what SetuHQ checks
| Quantity | Value | From |
|---|---|---|
| Kepler candidates that were false positives | 9.4% | overall; 17.7% for giants (Fressin et al. 2013) |
| TESS prime-mission TOIs found false by follow-up | 565 of 2,241 (≈25%) | Guerrero et al. 2021 |
| A 50% binary eclipse diluted 1,000 times | 500 ppm | δ_obs = δ_true · F_target/F_total [calc]: the depth of a small planet |
| pi Men c's shape, T23/T14 | 0.95 | flat-bottomed (U), not V [calc from the transit chapter] |
SetuHQ's vetting flags, from the light curve alone: odd_even_mismatch (odd and even depths differ), secondary_eclipse (a dip at phase 0.5), low_snr, too_short, edge_event and insufficient_points. It has no pixel-level centroid or difference-image check and no statistical validation, so a blended background binary can pass. See the reviewers › · See a vetted case ›