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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 2.

NIRB and NIRF realizations as in Figure 1, and the g − r, r − i and r − z colors and their respective uncertainties of the objects with p₀ < 0.001 for both components, and uncertainties <0.5 (<0.2) for the most (least) uncertain color. One of the outliers (in red) is Eris, and three of them in blue are potential Haumea-family members. The other outliers (in green) are marked individually in the panels.

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