Discovery of a warm, dusty giant planet around HIP 65426
Aims. The SHINE program is a high-contrast near-infrared survey of 600 young, nearby stars
aimed at searching for and characterizing new planetary systems using VLT/SPHERE's …
aimed at searching for and characterizing new planetary systems using VLT/SPHERE's …
Shadows and spirals in the protoplanetary disk HD 100453
M Benisty, T Stolker, A Pohl, J De Boer, G Lesur… - Astronomy & …, 2017 - aanda.org
Context. Understanding the diversity of planets requires studying the morphology and
physical conditions in the protoplanetary disks in which they form. Aims. We aim to study the …
physical conditions in the protoplanetary disks in which they form. Aims. We aim to study the …
Multiple disk gaps and rings generated by a single Super-Earth
We investigate the observational signatures of super-Earths (ie, planets with Earth-to-
Neptune mass), which are the most common type of exoplanet discovered to date, in their …
Neptune mass), which are the most common type of exoplanet discovered to date, in their …
orbitize!: A comprehensive orbit-fitting software package for the high-contrast imaging community
Abstract orbitize! is an open-source, object-oriented software package for fitting the orbits of
directly imaged objects. It packages the Orbits for the Impatient (OFTI) algorithm and a …
directly imaged objects. It packages the Orbits for the Impatient (OFTI) algorithm and a …
Direct imaging and astrometric detection of a gas giant planet orbiting an accelerating star
T Currie, GM Brandt, TD Brandt, B Lacy, A Burrows… - Science, 2023 - science.org
Direct imaging of gas giant exoplanets provides information on their atmospheres and the
architectures of planetary systems. However, few planets have been detected in blind …
architectures of planetary systems. However, few planets have been detected in blind …
The time domain for brown dwarfs and directly imaged giant exoplanets: the power of variability monitoring
B Biller - Astronomical Review, 2017 - Taylor & Francis
Variability has now been robustly observed in a range of L and T type field brown dwarfs,
primarily at near-IR and mid-IR wavelengths. The probable cause of this variability is surface …
primarily at near-IR and mid-IR wavelengths. The probable cause of this variability is surface …
Spectral and atmospheric characterization of 51 Eridani b using VLT/SPHERE
M Samland, P Mollière, M Bonnefoy, AL Maire… - Astronomy & …, 2017 - aanda.org
Context. 51 Eridani b is an exoplanet around a young (20 Myr) nearby (29.4 pc) F0-type star,
which was recently discovered by direct imaging. It is one of the closest direct imaging …
which was recently discovered by direct imaging. It is one of the closest direct imaging …
The VLT/NaCo large program to probe the occurrence of exoplanets and brown dwarfs at wide orbits-IV. Gravitational instability rarely forms wide, giant planets
Understanding the formation and evolution of giant planets (≥ 1 M Jup) at wide orbital
separation (≥ 5 AU) is one of the goals of direct imaging. Over the past 15 yr, many surveys …
separation (≥ 5 AU) is one of the goals of direct imaging. Over the past 15 yr, many surveys …
Direct detection of scattered light gaps in the transitional disk around HD 97048 with VLT/SPHERE
C Ginski, T Stolker, P Pinilla, C Dominik… - Astronomy & …, 2016 - aanda.org
Aims. We studied the well-known circumstellar disk around the Herbig Ae/Be star HD 97048
with high angular resolution to reveal undetected structures in the disk which may be …
with high angular resolution to reveal undetected structures in the disk which may be …
Observing exoplanets with high dispersion coronagraphy. I. The scientific potential of current and next-generation large ground and space telescopes
Direct imaging of exoplanets presents a formidable technical challenge owing to the small
angular separation and high contrast between exoplanets and their host stars. High …
angular separation and high contrast between exoplanets and their host stars. High …