2020
DOI: 10.1002/essoar.10504271.1
|View full text |Cite
Preprint
|
Sign up to set email alerts
|

Constraining the Densities of the Three Kepler-289 Planets with Transit Timing Variations

Abstract: Kepler-289 is a three-planet system containing two sub-Neptunes and one cool giant planet orbiting a young, Sun-like star. All three planets exhibit transit timing variations (TTVs), with both adjacent planet pairs having orbital periods close to the 2:1 orbital resonance. We observe two transits of Kepler-289c with the Wide-field InfraRed Camera (WIRC) on the 200" Hale Telescope at Palomar Observatory, using diffuser-assisted photometry to achieve space-like photometric precision from the ground. These new tr… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...

Citation Types

0
0
0

Publication Types

Select...

Relationship

0
0

Authors

Journals

citations
Cited by 0 publications
references
References 46 publications
0
0
0
Order By: Relevance

No citations

Set email alert for when this publication receives citations?