Distant Giants Survey Archives

Close-in small planets and their distant giant companions. Masses and periods of exoplanets from our survey (bold squares) and the NASA Exoplanet Archive (faded circles) for context . Red/blue points indicate planets discovered using the transit/RV method. Red squares show true masses of transiting planets in the Distant Giants Survey measured by RVs (Polanski et al. 2024), while blue squares show minimum mass measurements (M sin i). For systems with multiple transiting planets, we show the parameters of the transiting planet with the lowest TOI designation that passed our filters. Red squares with yellow borders indicate systems in which we detected a linear/quadratic trend. Giant planets in our sample are connected to the inner planet in their system by a black line. The box corresponds to our nominal definition of a Distant Giant. -- astro-ph.EP

Astronomy & Telescopes, Brown Dwarfs, Exoplanets, -moons, -comets, Exploration Gear & Tech, Gas Giants, Status Report, Stellar Cartography

The TESS-Keck Survey XXIV: Outer Giants May be More Prevalent in the Presence of Inner Small Planets

by Keith CowingJanuary 14, 2025January 14, 2025

We present the results of the Distant Giants Survey, a three-year radial velocity (RV) campaign to search for wide-separation giant planets orbiting Sun-like stars known to host an inner transiting […]

Distant Giants Survey

The TESS-Keck Survey XXIV: Outer Giants May be More Prevalent in the Presence of Inner Small Planets

Astrochemistry In Action: JWST View Of The Carina Nebula

Reconstructing Ancient Protein Alphabets: What Can We Truly Infer?

Inventories of Rich Carbon-Chain Chemistry in Prestellar and Starless Cores in the Perseus Molecular Cloud

Variations in the 3.3 µm Polycyclic Aromatic Hydrocarbon Feature Across Nearby Galaxies Driven by Metallicity and Radiation Field Spectrum

Exploration Of Exoplanet Atmospheres With The James Webb Space Telescope