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BANYAN. XI. The BANYAN Σ multivariate Bayesian algorithm to identify members of young associations with 150 pc
BANYAN Σ is a new Bayesian algorithm to identify members of young stellar associations
within 150 pc of the Sun. It includes 27 young associations with ages in the range∼ 1–800 …
within 150 pc of the Sun. It includes 27 young associations with ages in the range∼ 1–800 …
Debris disk results from the Gemini Planet Imager Exoplanet Survey's polarimetric imaging campaign
We report the results of a∼ 4 yr direct imaging survey of 104 stars to resolve and
characterize circumstellar debris disks in scattered light as part of the Gemini Planet Imager …
characterize circumstellar debris disks in scattered light as part of the Gemini Planet Imager …
DUst around NEarby Stars. The survey observational results
C Eiroa, JP Marshall, A Mora, B Montesinos… - Astronomy & …, 2013 - aanda.org
Context. Debris discs are a consequence of the planet formation process and constitute the
fingerprints of planetesimal systems. Their solar system counterparts are the asteroid and …
fingerprints of planetesimal systems. Their solar system counterparts are the asteroid and …
Probing for exoplanets hiding in dusty debris disks: disk imaging, characterization, and exploration with HST/STIS multi-roll coronagraphy
Spatially resolved scattered-light images of circumstellar debris in exoplanetary systems
constrain the physical properties and orbits of the dust particles in these systems. They also …
constrain the physical properties and orbits of the dust particles in these systems. They also …
SONS: The JCMT legacy survey of debris discs in the submillimetre
WS Holland, BC Matthews, GM Kennedy… - Monthly Notices of …, 2017 - academic.oup.com
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 …
their presence around stars also suggests that planets exist in these systems. In this paper …
Do two-temperature debris discs have multiple belts?
GM Kennedy, MC Wyatt - Monthly Notices of the Royal …, 2014 - academic.oup.com
We present a study of debris discs whose spectra are well modelled by dust emission at two
different temperatures. These discs are typically assumed to be a sign of multiple belts …
different temperatures. These discs are typically assumed to be a sign of multiple belts …
A statistical analysis of SEEDS and other high-contrast exoplanet surveys: Massive planets or low-mass brown dwarfs?
TD Brandt, MW McElwain, EL Turner… - The Astrophysical …, 2014 - iopscience.iop.org
We conduct a statistical analysis of a combined sample of direct imaging data, totalling
nearly 250 stars. The stars cover a wide range of ages and spectral types, and include five …
nearly 250 stars. The stars cover a wide range of ages and spectral types, and include five …
Lacewing: A new moving group analysis code
We present a new nearby young moving group (NYMG) kinematic membership analysis
code, LocAting Constituent mEmbers In Nearby Groups (LACEwING), a new Catalog of …
code, LocAting Constituent mEmbers In Nearby Groups (LACEwING), a new Catalog of …
The International Deep Planet Survey-II. The frequency of directly imaged giant exoplanets with stellar mass
R Galicher, C Marois, B Macintosh… - Astronomy & …, 2016 - aanda.org
Context. Radial velocity and transit methods are effective for the study of short orbital period
exoplanets but they hardly probe objects at large separations for which direct imaging can …
exoplanets but they hardly probe objects at large separations for which direct imaging can …
[HTML][HTML] Discovery of a low-mass companion inside the debris ring surrounding the F5V star HD 206893
Aims. Uncovering the ingredients and the architecture of planetary systems is a very active
field of research that has fuelled many new theories on giant planet formation, migration …
field of research that has fuelled many new theories on giant planet formation, migration …