Context. The Gaia DR3 catalogue contains, for the first time, about 800 000 solutions with
either orbital elements or trend parameters for astrometric, spectroscopic, and eclipsing …

The most direct and substantial way to measure the geochemistry of extrasolar objects is to
perform chemical autopsies on their broken-up remains. However, traditional ways of …

About ten percent of Sun-like (1–2 M⊙) stars will engulf a 1–10 MJ planet as they expand
during the red giant branch (RGB) or asymptotic giant branch (AGB) phase of their evolution …

Abstract The MIRI Exoplanets Orbiting White dwarfs survey is a cycle 2 JWST program to
search for exoplanets around dozens of nearby white dwarfs via infrared excess and direct …

We report the discovery of two directly imaged, giant planet candidates orbiting the metal-
rich, hydrogen atmosphere white dwarfs WD 1202− 232 and WD 2105− 82. JWST's Mid …

As the Kepler mission has done for hot exoplanets, the ESA Euclid and NASA Roman
missions have the potential to create a breakthrough in our understanding of the …

ABSTRACT A new class of white dwarfs, dubbed DAHe, that present Zeeman-split Balmer
lines in emission has recently emerged. However, the physical origin of these emission lines …

Two recently discovered white dwarfs, WD J041246. 84+ 754942.26 and WD J165335. 21−
100116.33, exhibit Hα and Hβ Balmer line emission similar to stars in the emerging DAHe …

ABSTRACT A large fraction of white dwarfs are accreting or have recently accreted rocky
material from their planetary systems, thereby 'polluting'their atmospheres with elements …

We demonstrate that the James Webb Space Telescope (JWST) can detect infrared (IR)
excess from the blended light spectral energy distribution of spatially unresolved terrestrial …