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GERBLS—A Rapid Box Least Squares Algorithm for Exoplanet Detection That Scales Well for Large Datasets

  • Authors: Kristo Ment, Eric B. Ford, Suvrath Mahadevan, Rachel B. Fernandes, Andrew Hotnisky

Kristo Ment et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 8.

Top: TESS PDCSAP light curve for TRAPPIST-1 from Observation Sector 70. The blue points represent valid data, while the red points were masked out during detrending. The orange line shows the fitted long-term flux baseline that was generated using an SG filter. The black and red triangle markers near the top denote the locations of transits of TRAPPIST-1 b and c, respectively, based on the limb-darkened transit models shown in Figure 10. Bottom: Flux residuals after dividing out the long-term flux baseline, binned to a 1 hr cadence. The rms of the unbinned residuals is 13.88 parts-per-thousand.

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