no code implementations • 10 Dec 2024 • J. Toivanen, V. Kolehmainen, A. Paldanius, A. Hänninen, A. Hauptmann, S. J. Hamilton
Results: Post-processing the linear difference reconstructions through the graph U-net significantly improved the image quality, resulting in images comparable to, or better than, the time-intensive nonlinear reconstruction method (a few minutes vs. several hours).
no code implementations • 10 Feb 2021 • K. J. Napier, D. W. Gerdes, Hsing Wen Lin, S. J. Hamilton, G. M. Bernstein, P. H. Bernardinelli, T. M. C. Abbott, M. Aguena, J. Annis, S. Avila, D. Bacon, E. Bertin, D. Brooks, D. L. Burke, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, M. Costanzi, L. N. da Costa, J. De Vicente, H. T. Diehl, P. Doel, S. Everett, I. Ferrero, P. Fosalba, J. García Bellido, D. Gruen, R. A. Gruendl, G. Gutierrez, D. L. Hollowood, K. Honscheid, B. Hoyle, D. J. James, S. Kent, K. Kuehn, N. Kuropatkin, M. A. G. Maia, F. Menanteau, R. Miquel, R. Morgan, A. Palmese, F. Paz-Chinchón, A. A. Plazas, E. Sanchez, V. Scarpine, S. Serrano, I. Sevilla-Noarbe, M. Smith, E. Suchyta, M. E. C. Swanson, C. To, A. R. Walker, R. D. Wilkinson
The apparent clustering in longitude of perihelion $\varpi$ and ascending node $\Omega$ of extreme trans-Neptunian objects (ETNOs) has been attributed to the gravitational effects of an unseen 5-10 Earth-mass planet in the outer solar system.
Selection bias
Earth and Planetary Astrophysics
no code implementations • 30 Nov 2018 • S. J. Hamilton, A. Hänninen, A. Hauptmann, V. Kolehmainen
This allows the training data to be boundary shape independent.