Astrometry and Occultation predictions to Trans-Neptunian and Centaur Objects observed within the Dark Energy Survey

Autor: V. Scarpine, Juan de Vicente, Marcelo Assafin, J. Carretero, Flavia Sobreira, Alex Drlica Wagner, S. Serrano, Nikolay Kuropatkin, E. Suchyta, Tim Abbot, Mathew Smith, I. Sevilla, Aurelio Carnero Rossell, Rodney S. Gomes, Josh Frieman, A. A. Plazas, G. Gutierrez, Josselin Desmars, Julio Camargo, Enrique Gaztanaga, Roberto Vieira-Martins, M. A. G. Maia, Juan Garcia-Bellido, Matias Carrasco Kind, Ramon Miquel, E. Buckley-Geer, Luiz N. da Costa, Emmanuel Bertin, Ricardo L. C. Ogando, D. L. Burke, Michael Schubnell, David J. James, David J. Brooks, J. Gschwend, S. Avila, Gary Bernstein, S. Allam, Robert A. Gruendl, Matheus Gysi, Felipe Menanteau, Pablo Fosalba, Molly E. C. Swanson, Christopher J. Davis, Will G. Hartley, Marcelle Soares-Santos, Devon L. Hollowood, Martin Banda-Huarca, Filipe B. Abdalla, Gregory Tarle, Daniel Gruen, Felipe Braga Ribas, D. W. Gerdes, Peter Doel, Thomas Diehl, K. Honscheid, Christopher J. Miller, S. Hamilton, William Wester, Kyler Kuehn, Carlos E. Cunha, E. J. Sanchez, K. Romer

Publikováno v: Dark Energy Survey Collaboration & Avila, S 2019, ' Astrometry and Occultation predictions to Trans-Neptunian and Centaur Objects observed within the Dark Energy Survey ', The Astrophysical Journal, vol. 157, no. 3, 120 . https://doi.org/10.3847/1538-3881/aafb37
Astron.J.
Astron.J., 2019, 157 (3), pp.120. ⟨10.3847/1538-3881/aafb37⟩
The Astronomical Journal

Transneptunian objects (TNOs) are a source of invaluable information to access the history and evolution of the outer solar system. However, observing these faint objects is a difficult task. As a consequence, important properties such as size and al

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