activity
20062026
most citedThe Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance

8k citations · 11.5k across the 73 of their papers we have counts for

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astro-ph.EP2026

COSINE (Cometary Object Study Investigating their Nature and Evolution) II: Colors and Sizes of Comet Nuclei

Yuna G. Kwon, Dar W. Dahlen, Joseph R. Masiero +6

Comet nuclei preserve a record of planetesimal formation, but their sizes are difficult to measure because the nucleus is usually blended with its coma. We present a catalog of nuc…

astro-ph.EP2025

NEOWISE data and Thermophysical Modeling of 98943 Torifune (2001 CC21)

Edward L., Wright, Jospeh Masiero +1

The Hayabusa2# flyby target 98943 Torifune (2001 CC21) has an uncertain size based on an uncertain albedo and uncertain absolute magnitude. We have collected all the NEOWISE observ…

astro-ph.EP2025

COSINE (Cometary Object Study Investigating their Nature and Evolution) I. Project Overview and General Characteristics of Detected Comets

Yuna G. Kwon, Dar W. Dahlen, Joseph R. Masiero +8

We present the first results from the COSINE (Cometary Object Study Investigating their Nature and Evolution) project, based on a uniformly processed dataset of 484 comets observed…

astro-ph.EP2024

Visual-band brightnesses of Near Earth Objects that will be discovered in the infrared by NEO Surveyor

Joseph R. Masiero, Tyler Linder, Amy Mainzer +2

NEO Surveyor will detect asteroids and comets using mid-infrared thermal emission, however ground-based followup resources will require knowledge of the expected visible light brig…

astro-ph.EP2024

The Sensitivity of NEO Surveyor to Low-Perihelion Asteroids

Joseph R. Masiero, Yuna G. Kwon, Dar W. Dahlen +2

Asteroids with low orbital perihelion distances experience extreme heating from the Sun that can modify their surfaces and trigger non-typical activity mechanisms. These objects ar…

astro-ph.EP2024

NEOWISE Observations of Distant Active Long-period Comets C/2014 B1 (Schwartz), C/2017 K2 (Pan-STARRS), and C/2010 U3 (Boattini)

Dave G. Milewski, Joseph R. Masiero, Jana Pittichova +3

Hyperactive comet activity typically becomes evident beyond the frost line (3 to 4 au) where it becomes too cold for water-ice to sublimate. If carbon monoxide (CO) and carbon diox…