SDSS-based taxonomic classification and orbital distribution of main belt asteroids

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The Compositional Structure of the Asteroid Belt (2015, background): “mation about the Asteroid Belt’s dynamic past. About 100,000 asteroids have measurements that tell us about their surface compositions (Ivezic et al., 2001, Szabo et al., 2004, Nesvorny et al., 2005, Carvano et al., 2010), providing a broader view of the Asteroid Belt than ever before. With the expl”
Compositional distributions and evolutionary processes for the near-Earth object population: Results from the MIT-Hawaii Near-Earth Object Spectroscopic Survey (MITHNEOS) (2019, methodology): “Solar System objects observed in the Sloan Digital Sky Survey commissioning data.”
The taxonomic distribution of asteroids from multi-filter all-sky photometric surveys (2013, background): “Carvano et al. (2010) converted colors to reflectance val-”
J-PLUS: The Javalambre Photometric Local Universe Survey (2015, methodology): “Although Article number, page 24 of 29 most asteroid taxonomical classes can be defined using intermediate band filters like the SDSS filter system (Carvano et al. 2010), the low spectral resolution tends to render the detection of the 0.7 µm band unreliable using SDSS data (Rivkin 2012).”