Image Details

Choose export citation format:

An Independent Search for Small Long-period Planets in Kepler Data. I. Detection Pipeline

  • Authors: Oryna Ivashtenko, Barak Zackay

Oryna Ivashtenko and Barak Zackay 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 2.

Schematic of data conditioning on a simulated light curve represented in Fourier domain. (1) The original correlated (red noise) flux, including an additional noise peak. (2) The flux after detrending the low frequencies that cannot be resolved by the measured PSD. (3) The flux whitened after the PSD was measured and the whitening filter was constructed. (4) The flux after the peak detection and removal. (5) The final whitened flux, which will be used for statistic score calculation.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse