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We tested whether explicit flare and artifact controls improve recovery of simulated stellar self-lensing pulses in public Transiting Exoplanet Survey Satellite (TESS) light curves. A preregistered sample contains 100 stars, with 40 used for development and 60 for evaluation. At the same empirical background-trigger fraction of 10%, the development-selected controls recovered 269 of 540 pulses (49.8%), versus 239 (44.3%) for the lensing-template baseline. The difference is 5.6 percentage points, with a paired target-bootstrap interval from -10.6 to 26.7 percentage points. This pilot leaves a recovery benefit unresolved. Background triggers are not labeled false alarms, and this study makes no astronomical discovery claim.
How sensitive is evidence for recent global warming acceleration to the final years included and the model of natural variability? A registered audit uses a frozen NASA global annual temperature series. A fixed-breakpoint model estimates a warming-rate increase of 0.232 °C per decade, with a confidence interval from 0.106 to 0.358. A search over possible breakpoints gives p = 0.0271 with fitted autocorrelation, but p = 0.4078 when the recent endpoint years are excluded. Stronger assumed autocorrelation also weakens the test. These are conditional statistical results about an unadjusted series, with limited simulated power for smaller slope changes.