Image Details

Choose export citation format:

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 2.

The period sampling of GERBLS. The blue line represents uniformly sampled orbital frequencies (frequency differential Δf = const.), whereas the green line shows a sampling that is uniform in orbital period (Δf ∝ P−2). GERBLS (solid black dots) natively produces a sampling that is broadly a combination of the two, with the frequency differential approximated by Δf ∝ P−1 (red line). Smaller jumps between frequencies occur when moving from one folding transform to the next (with a base period larger by 1). When automatic downsampling is switched on (orange dots), the frequency differential can be well approximated as Δf ∝ P−0.72, which is close to the optimal search resolution of Δf ∝ P−2/3 for planets on circular orbits as demonstrated by A. Ofir (2014).

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse