False positive probabilties for all Kepler Objects of Interest: 1284 newly validated planets and 428 likely false positives
arXiv:1605.02825 · doi:10.3847/0004-637X/822/2/86
Abstract
We present astrophysical false positive probability calculations for every Kepler Object of Interest (KOI)---the first large-scale demonstration of a fully automated transiting planet validation procedure. Out of 7056 KOIs, we determine that 1935 have probabilities <1% to be astrophysical false positives, and thus may be considered validated planets. 1284 of these have not yet been validated or confirmed by other methods. In addition, we identify 428 KOIs likely to be false positives that have not yet been identified as such, though some of these may be a result of unidentified transit timing variations. A side product of these calculations is full stellar property posterior samplings for every host star, modeled as single, binary, and triple systems. These calculations use 'vespa', a publicly available Python package able to be easily applied to any transiting exoplanet candidate.
arXiv comment20 pages, 8 figures. Published in ApJ. Instructions to reproduce results can be found at https://github.com/timothydmorton/koi-fpp
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- Non-transiting exoplanets as a means of understanding star-planet interactions in close-in systems
- Scaling K2. V. Statistical Validation of 60 New Exoplanets From K2 Campaigns 2-18
- Effects of Self-gravity on Mass-loss of the Post-impact Super-Earths
- The Occurrence-weighted Median Planets Discovered by Transit Surveys Orbiting Solar-type Stars and Their Implications for Planet Formation and Evolution
- ASTEP confirmation of a pair of long-period Jupiter-sized planets with extremely low densities transiting TOI-791
- GJ 238 b: A 0.57 Earth Radius Planet Orbiting an M2.5 Dwarf Star at 15.2 pc
- Simulations Predicting the Ability of Multi-Color Simultaneous Photometry to Distinguish TESS Candidate Exoplanets from False Positives
- Characterisation of starspot structure and differential rotation of Kepler-411
- Sensitivity of Dry Lava Planet Atmospheric Emission Spectra to Changes in Lava Compositions
- Simulation of the spin evolution of some selected exoplanets and inferences on their climate
- How to measure tidal dissipation in long resonant chains
- Comprehensive Parameter Determination of Exoplanet through Asteroseismic Host Star Constraints
- Kepler-1624b Has No Significant Transit Timing Variations
- Dynamics of Two Planets near a 2:1 Resonance: Case Studies of Known and Synthetic Exosystems on a Grid of Initial Configurations
- TFAW survey II: 6 Newly Validated Planets and 13 Planet Candidates from K2
- Transit modelling of selected Kepler systems
- Refining the Masses and Radii of the Star Kepler-33 and its Five Transiting Planets
- Constraints on the Obliquities of Kepler Planet-Hosting Stars
- The Dynamical Environment of Kepler-223 Planetary System
- Transit Hunt for Young and Maturing Exoplanets (THYME) VIII: a Pleiades-age association harboring two transiting planetary systems from Kepler
- The TESS-Keck Survey. XI. Mass Measurements for Four Transiting sub-Neptunes orbiting K dwarf TOI-1246
- The California Legacy Survey III. On The Shoulders of (Some) Giants: The Relationship between Inner Small Planets and Outer Massive Planets
- Do the planets in the HD 34445 system really exist?
- Exoplanet transit search at the detection limit: detection and false alarm vetting pipeline