Asteroid Catalog Using AKARI: AKARI/IRC Mid-Infrared Asteroid Survey

By F. Usui, D. Kuroda, T. Müller, S. Hasegawa, M. Ishiguro, T. Ootsubo, D. Ishihara, H. Kataza, S. Takita, S. Oyabu and 3 more. 2011

176 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

Density of asteroids (2012, background): “Among the C-complex, B-types have distinct surface properties: negative spectral slope in the visible and higher albedo (see the compilation of albedo per taxonomic class from Ryan and Woodward (2010); Usui et al. (2011); Masiero et al. (2011)).”
The taxonomic distribution of asteroids from multi-filter all-sky photometric surveys (2013, methodology): “n values, weighted by the number of albedos determined and their accuracy, for each taxonomic class for this work based on averages reported from previously published results (Ryan and Woodward 2010, Usui et al. 2011, Masiero et al. 2011). See Table 1 for a summary of published values and the averag”
Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations (2012, unknown): “…Satellite (IRAS) , the Wide-ﬁeld Infrared Survey Explorer (WISE) , AKARI and the Spitzer Space Telescope resulted in estimates of diameters and albedos for thousands of asteroids (e.g., Tedesco et al., 2002; Mainzer et al., 2011a,b; Masiero et al., 2011; Usui et al., 2011; Ryan and Woodward, 2011).”