activity
19952026
most citedThe Hawaii Infrared Parallax Program. I. Ultracool Binaries and the L/T Transition

572 citations · 13.9k across the 207 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.SRShow all

10 papers · 2 filters

astro-ph.SR2017★ 57 cited

Cloudless atmospheres for young low-gravity substellar objects

P. Tremblin, G. Chabrier, I. Baraffe +7

Atmospheric modeling of low-gravity (VL-G) young brown dwarfs remains a challenge. The presence of very thick clouds has been suggested because of their extremely red near-infrared…

astro-ph.SR2017★ 22 cited

The Multiplicity of M-Dwarfs in Young Moving Groups

Yutong Shan, Jennifer C. Yee, Brendan P. Bowler +11

We image 104 newly identified low-mass (mostly M-dwarf) pre-main sequence members of nearby young moving groups with Magellan Adaptive Optics (MagAO) and identify 27 binaries with…

astro-ph.SR2017★ 106 cited

All-sky Co-moving Recovery Of Nearby Young Members. (ACRONYM) II: The Beta Pictoris Moving Group

Evgenya L. Shkolnik, Katelyn N. Allers, Adam L. Kraus +2

We confirm 66 low-mass stellar and brown dwarf systems (K7-M9) plus 19 visual or spectroscopic companions of the beta Pictoris Moving Group (BPMG). Of these, 41 are new discoveries…

astro-ph.SR2017★ 58 cited

The Young L Dwarf 2MASS J11193254-1137466 is a Planetary-Mass Binary

William M. J. Best, Michael C. Liu, Trent J. Dupuy +1

We have discovered that the extremely red, low-gravity L7 dwarf 2MASS J11193254-1137466 is a 0.14" (3.6 AU) binary using Keck laser guide star adaptive optics imaging. 2MASS J11193…

astro-ph.SR2017★ 8 cited

CFBDSIR 2149-0403: young isolated planetary-mass object or high-metallicity low-mass brown dwarf??

P. Delorme, T. Dupuy, J. Gagné +12

We conducted a multi-wavelength, multi-instrument observational characterisation of the candidate free-floating planet CFBDSIR~J214947.2-040308.9, a late T-dwarf with possible low-…

astro-ph.SR2017★ 199 cited

Individual Dynamical Masses of Ultracool Dwarfs

Trent J. Dupuy, Michael C. Liu

We present the full results of our decade-long astrometric monitoring programs targeting 31 ultracool binaries with component spectral types M7-T5. Joint analysis of resolved imagi…