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 apply the vectorized non-negative matrix factorization (NMF) method to the post-
processing of the direct imaging data of exoplanetary systems such as circumstellar disks …

ABSTRACT A new class of high-contrast image analysis algorithms that empirically fit and
subtract systematic noise has lead to recent discoveries of faint exoplanet/substellar …

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 …

We present optical and near-infrared high-contrast images of the transitional disk HD
100546 taken with the Magellan Adaptive Optics system (MagAO) and the Gemini Planet …

We present the first scattered light detections of the HD 106906 debris disk using the
Gemini/Gemini Planet Imager in the infrared and Hubble Space Telescope (HST)/Advanced …

ABSTRACT A" minimum model" for debris disks consists of a narrow ring of parent bodies,
secularly forced by a single planet on a possibly eccentric orbit, colliding to produce dust …

Context. HD 106906AB is the only young binary system so far around which a planet has
been imaged and a debris disk has been shown to exist, thanks to a strong IR excess. As …

Context. Debris disks offer valuable insights into the latest stages of circumstellar disk
evolution, and can possibly help us to trace the outcomes of planetary formation processes …

Abstract We present Atacama Large Millimeter/submillimeter Array (ALMA) 1.3 mm (230
GHz) observations of the HD 32297 and HD 61005 debris disks, two of the most iconic …