View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Caltech Authors The Astrophysical Journal, 791:121 (11pp), 2014 August 20 doi:10.1088/0004-637X/791/2/121 C 2014. The American Astronomical Society. All rights reserved. Printed in the U.S.A. MAIN-BELT ASTEROIDS WITH WISE/NEOWISE: NEAR-INFRARED ALBEDOS Joseph R. Masiero1, T. Grav2, A. K. Mainzer1,C.R.Nugent1,J.M.Bauer1,3, R. Stevenson1, and S. Sonnett1 1 Jet Propulsion Laboratory/Caltech, 4800 Oak Grove Drive, MS 183-601, Pasadena, CA 91109, USA;
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[email protected] 3 Infrared Processing and Analysis Center, Caltech, Pasadena, CA, USA Received 2014 May 14; accepted 2014 June 25; published 2014 August 6 ABSTRACT We present revised near-infrared albedo fits of 2835 main-belt asteroids observed by WISE/NEOWISE over the course of its fully cryogenic survey in 2010. These fits are derived from reflected-light near-infrared images taken simultaneously with thermal emission measurements, allowing for more accurate measurements of the near- infrared albedos than is possible for visible albedo measurements. Because our sample requires reflected light measurements, it undersamples small, low-albedo asteroids, as well as those with blue spectral slopes across the wavelengths investigated. We find that the main belt separates into three distinct groups of 6%, 16%, and 40% reflectance at 3.4 μm.