BANYAN. XI. The BANYAN Σ multivariate Bayesian algorithm to identify members of young associations with 150 pc

J Gagné, EE Mamajek, L Malo, A Riedel… - The Astrophysical …, 2018 - iopscience.iop.org
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 …

Debris disk results from the Gemini Planet Imager Exoplanet Survey's polarimetric imaging campaign

TM Esposito, P Kalas, MP Fitzgerald… - The Astronomical …, 2020 - iopscience.iop.org
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 …

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 …

Probing for exoplanets hiding in dusty debris disks: disk imaging, characterization, and exploration with HST/STIS multi-roll coronagraphy

G Schneider, CA Grady, DC Hines… - The Astronomical …, 2014 - iopscience.iop.org
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 …

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 …

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 …

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 …

Lacewing: A new moving group analysis code

AR Riedel, SC Blunt, EL Lambrides… - The Astronomical …, 2017 - iopscience.iop.org
We present a new nearby young moving group (NYMG) kinematic membership analysis
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 …

[HTML][HTML] Discovery of a low-mass companion inside the debris ring surrounding the F5V star HD 206893

J Milli, P Hibon, V Christiaens, É Choquet… - Astronomy & …, 2017 - aanda.org
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 …