Debris disks are tenuous, dust-dominated disks commonly observed around stars over a
wide range of ages. Those around main sequence stars are analogous to the Solar System's …

We know little about the outermost exoplanets in planetary systems because our detection
methods are insensitive to moderate-mass planets on wide orbits. However, debris discs …

Debris discs are evidence of the ongoing destructive collisions between planetesimals, and
their presence around stars also suggests that planets exist in these systems. In this paper …

Resolved observations of millimeter-sized dust, tracing larger planetesimals, have
pinpointed the location of 26 Edgeworth–Kuiper Belt analogs. We report that a belt's …

Abstract The Hunt for Observable Signatures of Terrestrial Systems survey searches for dust
near the habitable zones (HZs) around nearby, bright main-sequence stars. We use nulling …

We present the most sensitive direct imaging and radial velocity (RV) exploration of epsilon
Eridani to date. epsilon Eridani is an adolescent planetary system, reminiscent of the early …

The exoplanetary system of HR 8799 is one of the rare systems in which multiple planets
have been directly imaged. Its architecture is strikingly similar to that of the solar system, with …

Abstract epsilon Eridani is a young planetary system hosting a complex multibelt debris disk
and a confirmed Jupiter-like planet orbiting at 3.48 au from its host star. Its age and …

The excess emission seen in spectral energy distributions (SEDs) is commonly used to infer
the properties of the emitting circumstellar dust in protoplanetary and debris discs. Most …

With its near-to-mid-infrared high-contrast imaging capabilities, JWST is ushering us into a
golden age of directly imaging Jupiter-like planets. As the two closest cold Jupiters, ε Ind A b …