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Astronomical Image Time Series Segmentation for Faint, Fast Object Detection

  • Authors: Dan Caselden, J. Davy Kirkpatrick, Lindsey Lack, Andrew White, Federico Marocco, Aaron M. Meisner, Guillaume Colin, Bruce Baller, Kareem Ammar, Thomas P. Bickle, Hunter Brooks, S. L. Casewell, Peter R. M. Eisenhardt, Charles A. Elachi, Jacqueline K. Faherty, John W. Fowler, Daniella C. Bardalez Gagliuffi, Jonathan Gagné, Christopher R. Gelino, Jake Grigorian, Les Hamlet, Hiro Higashimura, 村滉 東, Justin Hong, Issam Ibnouhsein, Tarun Kota, Marc J. Kuchner, Ken A. Marsh, Matteo Paz, Yadukrishna Raghu, Adam C. Schneider, Sajesh Singh, Asa Trek, Kieran Wall, Andrew Washburn, Edward L. Wright, David Zurek

Dan Caselden et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 8.

Histograms comparing the number of fast (﹩\mu \geqslant 0\mathop{.}\limits^{^{\prime\prime} }35\,{\mathrm{yr}}^{-1}﹩) objects detected by SMDET (magenta line) and other WISE searches (blue areas). W2 reduced proper motion (top) and W2 apparent magnitude (bottom) are on the x-axes, with the number of objects per bin on the y-axes. All series are overplotted—not stacked. K = J. D. Kirkpatrick et al. (2014, 2016), S = A. C. Schneider et al. (2016), L = K. L. Luhman (2014), M = A. M. Meisner et al. (2020a, 2020b).

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