activity
19982023
most citedInitial Performance of the NEOWISE Reactivation Mission

764 citations · 15.9k across the 158 of their papers we have counts for

collaborators

159 papers

astro-ph.SR2023★ 2 cited

Young Stellar Object Candidates in IC 417

L. M. Rebull, R. L. Anderson, G. Hall +12

IC 417 is in the Galactic Plane, and likely part of the Aur OB2 association; it is ~2 kpc away. Stock 8 is one of the densest cluster constituents; off of it to the East, there is…

astro-ph.SR2023★ 6 cited

Long-term 4.6m Variability in Brown Dwarfs and a New Technique for Identifying Brown Dwarf Binary Candidates

Hunter Brooks, J. Davy Kirkpatrick, Aaron M. Meisner +11

Using a sample of 361 nearby brown dwarfs, we have searched for 4.6m variability indicative of large-scale rotational modulations or large-scale long-term changes on timescales…

astro-ph.SR2023★ 33 cited

JWST/NIRCam discovery of the first Y+Y brown dwarf binary: WISE J033605.05014350.4

Per Calissendorff, Matthew De Furio, Michael Meyer +25

We report the discovery of the first brown dwarf binary system with a Y dwarf primary, WISE J033605.05014350.4, observed with NIRCam on JWST with the F150W and F480M filters. We…

astro-ph.SR2023★ 20 cited

Redder than Red: Discovery of an Exceptionally Red L/T Transition Dwarf

Adam C. Schneider, Adam J. Burgasser, Justice Bruursema +26

We present the discovery of CWISE J050626.96073842.4 (CWISE J05060738), an L/T transition dwarf with extremely red near-infrared colors discovered through the Backyard Worlds…

astro-ph.SR2022

Discovery of 34 low-mass comoving systems using NOIRLab Source Catalog DR2

Frank Kiwy, Jacqueline K. Faherty, Aaron Meisner +14

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

astro-ph.SR2022★ 9 cited

CWISE J014611.20-050850.0AB: The Widest Known Brown Dwarf Binary in the Field

Emma Softich, Adam C. Schneider, Jennifer Patience +19

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 s…