activity
20082026
most citedOSSOS. VII. 800+ trans-Neptunian objects - the complete data release

159 citations · 1k across the 37 of their papers we have counts for

collaborators

37 papers

astro-ph.EP2026

Col-OSSOS: Investigating the Origins of Different Surfaces in the Primordial Kuiper Belt

Laura E. Buchanan, Megan E. Schwamb, Wesley C. Fraser +12

The Colours of the Outer Solar System Origins Survey (Col-OSSOS) measured the optical/NIR colours of a brightness-complete sample of Trans-Neptunian Objects (TNOs). Like previous s…

astro-ph.EP2025

LiDO: Discovery of a 10:1 Resonator with a Novel Libration State

Rosemary E. Pike, Ruth Murray-Clay, Kathryn Volk +9

The Large inclination Distant Objects LiDO survey has discovered the first securely classified object in the 10:1 mean motion resonance of Neptune. This object, 2020 VN40, is short…

astro-ph.EP2025★ 6 cited

Discovery and dynamics of a Sedna-like object with a perihelion of 66 au

Ying-Tung Chen, Patryk Sofia Lykawka, Yukun Huang +30

Trans-Neptunian objects (TNOs) with large perihelion distances ( au) and semi-major axes ( au) provide insights into the early evolution of the solar system and th…

astro-ph.EP2025

The Surfaces of Small to Mid-Size Plutinos: Evidence of an Association Between Inclination and Surface Type

Cameron Collyer, Rosemary E. Pike, Ying-Tung Chen +6

Being one of the most populated mean motion resonances (MMR) with Neptune and lying close to the inner boundary of the present day cold classical disk, observations of the orbital…

astro-ph.EP2025

LiDO: Exploring the Stable Plutino Parameter Space

Samantha M. Lawler, Mark Comte, Rosemary E. Pike +7

We present a publicly available, high-resolution, filled-parameter-space synthetic distribution of the Plutinos, trans-Neptunian Objects (TNOs) librating in the 3:2 mean-motion res…

astro-ph.EP2024

Small Bodies in the Distant Solar System

Samantha M. Lawler, Rosemary E. Pike

The small bodies in the Kuiper Belt region of the distant Solar System are leftovers from planet formation. Their orbital distribution today tells us about how giant planets migrat…