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Improving Exoplanet Detection Power: Multivariate Gaussian Process Models for Stellar Activity
David E. Jones, David C. Stenning, Eric B. Ford +4
The radial velocity method is one of the most successful techniques for detecting exoplanets. It works by detecting the velocity of a host star induced by the gravitational effect…
Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog With Measured Completeness and Reliability Based on Data Release 25
Susan E. Thompson, Jeffrey L. Coughlin, Kelsey Hoffman +58
We present the Kepler Object of Interest (KOI) catalog of transiting exoplanets based on searching four years of Kepler time series photometry (Data Release 25, Q1-Q17). The catalo…
Exploring Other Worlds: Science Questions for Future Direct Imaging Missions (EXOPAG SAG15 Report)
Daniel Apai, Nicolas Cowan, Ravikumar Kopparapu +30
The NASA Exoplanet Exploration Program's SAG15 group has solicited, collected, and organized community input on high-level science questions that could be addressed with future dir…
Insights on the Spectral Signatures of Stellar Activity and Planets from PCA
Allen B. Davis, Jessi Cisewski, Xavier Dumusque +2
Photospheric velocities and stellar activity features such as spots and faculae produce measurable radial velocity signals that currently obscure the detection of sub-meter-per-sec…
Evidence for Two Hot Jupiter Formation Paths
Benjamin E. Nelson, Eric B. Ford, Frederic A. Rasio
Disk migration and high-eccentricity migration are two well-studied theories to explain the formation of hot Jupiters. The former predicts that these planets can migrate up until t…
Outer Architecture of Kepler-11: Constraints from Coplanarity
Daniel Jontof-Hutter, Brian P. Weaver, Eric B. Ford +2
The outer architectures of Kepler's compact systems of multiple transiting planets remain poorly constrained and few of these systems have lower bounds on the orbital distance of a…