UMI: GPU-Accelerated Asymmetric Robust Estimator for Photometric Detrending in Exoplanet Transit Searches
Omar Khan

TL;DR
UMI is a GPU-accelerated robust estimator for photometric detrending in exoplanet transit searches, improving speed and accuracy especially at detectable transit depths.
Contribution
It introduces a novel asymmetric robust estimator, UMI, optimized with GPU acceleration, significantly enhancing transit detection performance over existing methods.
Findings
UMI achieves 69x faster detrending than previous implementations.
At 0.1% transit depth, UMI reduces median recovery error by up to 71%.
Validated on 802 confirmed exoplanets, UMI improves speed-accuracy tradeoff.
Abstract
We present UMI (Unified Median Iterative), a novel robust location estimator for detrending photometric time series in exoplanet transit surveys. UMI modifies the standard Tukey bisquare M-estimator with two innovations: (1) an asymmetric weight function that penalizes downward deviations (transit dips) more aggressively than upward ones, exploiting the physical constraint that transits are always below the stellar continuum, and (2) an upper-RMS scale estimator computed from above-median residuals only, ensuring that transit dips never contaminate the noise estimate. Implemented as a fused HIP/CUDA GPU kernel, UMI achieves 69x faster detrending (3.4 ms vs 234 ms per star) and 37x faster full pipeline throughput compared to the wotan biweight implementation. Injection-recovery tests across TESS, Kepler, and K2 show that UMI's advantage is concentrated at planet-scale transit depths…
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