119 citations · 2k across the 65 of their papers we have counts for
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Non-Vestoid candidate asteroids in the inner main belt
Dagmara Oszkiewicz, Brian A. Skiff, Nick Moskovitz +5
Most Howardite-Eucrite-Diogenite (HED) meteorites (analogs to V-type asteroids) are thought to originate from asteroid (4) Vesta. However, some HEDs show distinct oxygen isotope ra…
Physical Characterization of ~2-meter Diameter Near-Earth Asteroid 2015 TC25: A possible boulder from E-type Asteroid (44) Nysa
Vishnu Reddy, Juan A. Sanchez, William F. Bottke +11
Small near-Earth asteroids (>20 meters) are interesting because they are progenitors for meteorites in our terrestrial collection. Crucial to our understanding of the effectiveness…
Near-infrared thermal emission from near-Earth asteroids: Aspect-dependent variability
Nicholas A. Moskovitz, David Polishook, Francesca E. DeMeo +6
Here we explore a technique for constraining physical properties of near-Earth asteroids (NEAs) based on variability in thermal emission as a function of viewing aspect. We present…
Rotational properties of the Haumea family members and candidates: Short-term variability
Audrey Thirouin, Scott S. Sheppard, Keith S. Noll +3
Haumea is one of the most interesting and intriguing transneptunian objects (TNOs). It is a large, bright, fast rotator, and its spectrum indicates nearly pure water ice on the sur…
First Results from the Rapid-Response Spectrophotometric Characterization of Near-Earth Objects using UKIRT
M. Mommert, D. E. Trilling, D. Borth +7
Using the Wide Field Camera for the United Kingdom Infrared Telescope, we measure the near-infrared colors of near-Earth objects (NEOs) in order to put constraints on their taxonom…