Pedro Bernardinelli

@pbernardinelli.com

144 Followers 154 Following

Professor of astronomy @ University of São Paulo, PhD from Penn, formerly at UW. Discoverer of minor planets and C/2014 UN271, Brazilian, coffee dependent, geek. He/him/ele, pt-br/en

Fig 4 from the quoted paper

Table 4, showing the per-class population estimates

Posterior distributions of the inclination concentration parameter as a function of color and dynamical class

Figure 10, ternary diagram of occupation on the NIRB, as well as the redder and bluer halves of NIRB for the HCs, detached, and scattering objects

Figure 8. As before, but in bins of inclination

Figure 7, showing posteriors of NIRB occupation percentage per TNO dynamical class

figure 9, showing the data and the cumulative H mag distribution for six different TNO dynamical classes

Posterior samples for the LCA distribution, and the LCA distribution itself. Figure 6 from the paper

Equation 8, a Poisson likelihood for a general mixture model in TNO colors, sizes, lightcurves and orbital elements

Equation A8: a mixture model likelihood penalized by a selection function

Diagram of semi-major axes, eccentricities and inclination for all DES TNOs, color-coded by their color assignment and with symbols indicating dynamical class

Figure 1 of the paper, showing 800+ colors and the result Gaussian mixture model