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Rotational Light-curve Recovery and Predictions of the LSST Yield of Hildas

  • Authors: Alexander J. Fleming, Jacob A. Kurlander, Dmitrii E. Vavilov, David Vokrouhlický, David Nesvorný, Pedro H. Bernardinelli, Mario Jurić

Alexander J. Fleming et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 2.

Distribution of our 485,807 simulated Hildas projected onto 2D planes of their proper orbital parameters. (i) (a), (e) top left; (ii) (a, ﹩\sin (i)﹩) bottom left; and (iii) (e, ﹩\sin (i)﹩) bottom right. Each dark point represents an object from our simulated Hilda population. Approximate locations of the two largest collisional families associated with (153) Hilda (blue marker) and (1911) Schubart (red marker) are indicated for reference (D. Vokrouhlický et al. 2025).

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