Kepler-37 Archives

We include a variety of plots summarizing our training and analysis of HD 173701. Top Left: Kepler and TESS training data, as well as our best fit GP model overlaid. Top Right: RV time series and training posteriors. Bottom: Results of our injection-recovery analysis in the two cases described in §4. The left plots show the preference for models including the injected planet when no GP training is applied. The middle two plots show the improvements gained when training on Kepler or TESS. The rightmost plots highlight the differences between Kepler and TESS training. --astro-ph.EP

Astronomy & Telescopes, Exoplanets, -moons, -comets, Imaging & Spectroscopy, Status Report

Leveraging Precise Photometry From Kepler and TESS to Extract Exoplanets from Radial Velocity Time Series

by Keith CowingDecember 18, 2024December 18, 2024

Stellar activity contamination of radial velocity (RV) data is one of the top challenges plaguing the field of extreme precision RV (EPRV) science. Previous work has shown that photometry can […]

Kepler-37

Leveraging Precise Photometry From Kepler and TESS to Extract Exoplanets from Radial Velocity Time Series

A Proposal To Make Mars Sample Return A Collaborative NASA, ESA, And CNSA Effort

Planetary Research Program Metrics to Enable a Vital Research Community and Achieve Decadal-Level Science

NASA Spaceline Current Awareness List #1,220 9 October 2026 (Space Life Science Research Results)

Designing Protein Structures From Natural Language

How Long Could Volcanic Plumes Persist In The Venus Atmosphere?