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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 9.

Each panel shows the 68% limits of the data distributions per dynamical class (black) as well as the best-fit p(H_r) distribution multiplied by the selection function for the corresponding dynamical subset (red). In all cases, the data distribution has been constructed by sampling independent realizations of the H_r for each object, while the model distribution samples from the posterior of the likelihood.

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