adsabs/AstroCLIMB huggingface dataset:
Paper: Radar Circular Polarization Ratio of Near-Earth Asteroids: Links to Spectral Taxonomy and Surface Processes
Authors: Edgard G. Rivera-Valentín, Betzaida Aponte-Hernández, Patrick A. Taylor, Michael C. Nolan, Ellen S. Howell, Dany Waller, Luisa F. Zambrano-Marín, Anne K. Virkki, Ronald-Louis Ballouz, Angela M. Stickle
Figure caption: The standard deviation of CPR as a function of (a) rotation period and (b) absolute magnitude (H mag). Each colored point represents an iteration over a constant number of bins, following the color bar. The black dashed black line denotes the standard deviation of the entire data set for reference. Note that for (b) the x-axis is reversed to range from high to low absolute magnitude (i.e., from small to large objects).
Paper: Radar Circular Polarization Ratio of Near-Earth Asteroids: Links to Spectral Taxonomy and Surface Processes
Authors: Edgard G. Rivera-Valentín, Betzaida Aponte-Hernández, Patrick A. Taylor, Michael C. Nolan, Ellen S. Howell, Dany Waller, Luisa F. Zambrano-Marín, Anne K. Virkki, Ronald-Louis Ballouz, Angela M. Stickle
Figure caption: Fraction of NEAs with a given CPR belonging to the S and C complexes, as well as Q and L types, the X complex, and V-type asteroids, following the colors in the legend. The filled-in envelope represents the 1σ uncertainty. Transparency was added to facilitate simultaneously viewing the three uncertainty envelopes.
Paper: Radar Circular Polarization Ratio of Near-Earth Asteroids: Links to Spectral Taxonomy and Surface Processes
Authors: Edgard G. Rivera-Valentín, Betzaida Aponte-Hernández, Patrick A. Taylor, Michael C. Nolan, Ellen S. Howell, Dany Waller, Luisa F. Zambrano-Marín, Anne K. Virkki, Ronald-Louis Ballouz, Angela M. Stickle
Figure caption: Comparison of the PDF for NEAs with P < 2.4 hr and H mag > 23.5 (i.e., small and rapidly rotating) and P > 3.6 hr and H mag < 20 (i.e., large and slowly rotating). Each population is denoted by color following the legend, within which N is the total number of objects used to form the PDF. The filled-in space is the 1σ uncertainty envelope. Transparency was added to facilitate viewing of the PDFs simultaneously.
Paper: Radar Circular Polarization Ratio of Near-Earth Asteroids: Links to Spectral Taxonomy and Surface Processes
Authors: Edgard G. Rivera-Valentín, Betzaida Aponte-Hernández, Patrick A. Taylor, Michael C. Nolan, Ellen S. Howell, Dany Waller, Luisa F. Zambrano-Marín, Anne K. Virkki, Ronald-Louis Ballouz, Angela M. Stickle
Figure caption: Heat map of the resultant Wilcoxon rank-sum test for the (a) raw data and (b) 1σ upper confidence values using bootstrap methods for each of the studied taxonomic classes. Each p-value is annotated in the figure and noted by the color bar, where p ≤ 0.1 indicates evidence suggestive of differences in median values.