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Photometry of Outer Solar System Objects from the Dark Energy Survey. II. A Joint Analysis of Trans-Neptunian Absolute Magnitudes, Colors, Light Curves and Dynamics

Authors: Pedro H. Bernardinelli, Gary M. Bernstein, T. M. C. Abbott, M. Aguena, S. S. Allam, D. Brooks, A. Carnero Rosell, J. Carretero, L. N. da Costa, M. E. S. Pereira, T. M. Davis, J. De Vicente, S. Desai, H. T. Diehl, P. Doel, S. Everett, B. Flaugher, J. Frieman, J. García-Bellido, E. Gaztanaga, R. A. Gruendl, G. Gutierrez, K. Herner, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. J. James, K. Kuehn, O. Lahav, S. Lee, J. L. Marshall, J. Mena-Fernández, R. Miquel, J. Myles, A. A. Plazas Malagón, S. Samuroff, E. Sanchez, B. Santiago, I. Sevilla-Noarbe, M. Smith, E. Suchyta, G. Tarle, D. L. Tucker, V. Vikram, A. R. Walker, N. Weaverdyck

Pedro H. Bernardinelli et al 2025 The Astronomical Journal 169 .

Provider: AAS Journals

Caption: Figure 4.

The 68% and 95% posterior contours for the HMC-derived samples for the NIRB (left) and NIRF (right) parameters ﹩\bar{A}﹩ and s parameters of the LCA distribution. Each figure contains the posterior for all disjoint sets of objects from the distinct dynamical classes, and the posterior derived from fitting all the subsets simultaneously (the smallest, orange contours). Note there is no CC constraint on the NIRB component because the CCs are purely NIRF.

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