TESS Observations of Kepler systems with Transit Timing Variations
arXiv:2207.08917 · doi:10.3847/1538-3881/ac7396
Abstract
We identify targets in the Kepler field that may be characterized by transit timing variations (TTVs) and are detectable by the Transiting Exoplanet Survey Satellite (TESS). Despite the reduced signal-to-noise ratio of TESS transits compared to Kepler, we recover 48 transits from 13 systems in Sectors 14, 15, 26, 40 and 41. We find strong evidence of a nontransiting perturber orbiting Kepler-396 (KOI-2672) and explore two possible cases of a third planet in that system that could explain the measured transit times. We update the ephemerides and mass constraints where possible at KOI-70 (Kepler-20), KOI-82 (Kepler-102), KOI-94 (Kepler-89), KOI-137 (Kepler-18), KOI-244 (Kepler-25), KOI-245 (Kepler-37), KOI-282 (Kepler-130), KOI-377 (Kepler-9), KOI-620 (Kepler-51), KOI-806 (Kepler-30), KOI-1353 (Kepler-289) and KOI-1783 (Kepler-1662).
26 pages, 9 figures
References in corpus (20)
- The Transiting Exoplanet Survey Satellite
- DHP Framework: Digital Health Passports Using Blockchain -- Use case on international tourism during the COVID-19 pandemic
- The Mass of KOI-94d and a Relation for Planet Radius, Mass, and Incident Flux
- Spitzer Secondary Eclipses of the Dense, Modestly-irradiated, Giant Exoplanet HAT-P-20b Using Pixel-Level Decorrelation
- Planetary Candidates Observed by Kepler VI: Planet Sample from Q1-Q16 (47 Months)
- EVEREST: Pixel Level Decorrelation of K2 Light curves
- Alignment of the stellar spin with the orbits of a three-planet system
- Planetary Candidates Observed by Kepler V: Planet Sample from Q1-Q12 (36 Months)
- The Gaia-Kepler Stellar Properties Catalog. II. Planet Radius Demographics as a Function of Stellar Mass and Age
- The Featureless Transmission Spectra of Two Super-Puff Planets
- A 1.9 Earth radius rocky planet and the discovery of a non-transiting planet in the Kepler-20 system
- Planet Hunters VII. Discovery of a New Low-Mass, Low-Density Planet (PH3 c) Orbiting Kepler-289 with Mass Measurements of Two Additional Planets (PH3 b and d)
- The Compositional Diversity of Low-Mass Exoplanets
- The TESS-Keck Survey I: A Warm Sub-Saturn-mass Planet and a Caution about Stray Light in TESS Cameras
- The TESS-Keck Survey. VIII. Confirmation of a Transiting Giant Planet on an Eccentric 261 day Orbit with the Automated Planet Finder Telescope
- Eccentric Companions to Kepler-448b and Kepler-693b: Clues to the Formation of Warm Jupiters
- Spitzer Detection of the Transiting Jupiter-analog Exoplanet Kepler-167e
- No Timing Variations Observed in Third Transit of Snow-Line Exoplanet Kepler-421b
- Revisiting the Kepler field with TESS: Improved ephemerides using TESS 2min data
- Uniform Modeling of KOIs: MCMC Data Release Notes