Kepler Project Document: KSCI-19101 Planet Detection Metrics: Window and 1sigma Depth Functions for DR25

https://doi.org/10.26133/NEA28
https://www.ipac.caltech.edu/doi/10.26133/NEA28

10.26133/NEA28

IPAC

Kepler Project

Kepler Project Document: KSCI-19101 Planet Detection Metrics: Window and 1sigma Depth Functions for DR25

This document describes the window and one-sigma depth functions relevant to the Transiting Planet Search (TPS) algorithm in the Kepler pipeline. The window function specifies the fraction of unique orbital ephemeris epochs over which three transits are observable as a function of orbital period. In this context, the epoch and orbital period, together, comprise the ephemeris of an orbiting companion, and ephemerides with the same period are considered equivalent if their epochs differ by an integer multiple of the period. The one-sigma depth function specifies the depth of a signal (in ppm) for a given light curve that results in a one-sigma detection of a transit signature as a function of orbital period when averaged over all unique orbital ephemerides.

This dataset or service is made available by the NASA Exoplanet Science Institute at IPAC, which is operated by the California Institute of Technology under contract with the National Aeronautics and Space Administration.

Text

https://exoplanetarchive.ipac.caltech.edu/docs/KSCI-19101-002.pdf

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03 May 2017

2021