We present the positions, proper motions, and near-infrared photometry for 966 known
objects with spectral types later than M that were observed as part of the the UKIRT …

We present results from an atmospheric retrieval analysis of Gl 229B using the Brewster
retrieval code. We find the best fit model to be cloud-free, consistent with the T dwarf retrieval …

We present the projected rotational velocity and molecular abundances for HD 33632 Ab
obtained via Keck Planet Imager and Characterizer (KPIC) high-resolution spectroscopy. HD …

We present results from conducting a theoretical chemical analysis of a sample of
benchmark companion brown dwarfs whose primary star is of type F, G, or K. We summarize …

While stars are often found in binary systems, brown dwarf binaries are much rarer. Brown
dwarf–brown dwarf pairs are typically difficult to resolve because they often have very small …

We present the discovery of CWISE J050626. 96+ 073842.4 (CWISE J0506+ 0738), an L/T
transition dwarf with extremely red near-infrared colors discovered through the Backyard …

At the lowest masses, the distinction between brown dwarfs and giant exoplanets is often
blurred and literature classifications rarely reflect the deuterium burning boundary …

We present the discovery of 34 comoving systems containing an ultracool dwarf found by
means of the NOIRLab Source Catalog (NSC) DR2. NSC's angular resolution of∼ 1''allows …

Aims. We intended to quantify the impact of stellar multiplicity on the presence and
properties of exoplanets. Methods. We investigated all exoplanet host stars at less than 100 …

We present three new brown dwarf spectral-binary candidates: CWISE J072708. 09−
360729.2, CWISE J103604. 84− 514424.4, and CWISE J134446. 62− 732053.9, discovered …