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heliostack: A Novel Approach to Minor Planet Discovery

  • Authors: Kevin J. Napier, Matthew J. Holman, Hsing Wen Lin, 省文 林, David W. Gerdes, Thomas R. Ruch

Kevin J. Napier et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 2.

Top: distribution of the signal-to-noise ratio of all of the unique candidate trajectories resulting from the heliostack search, with ν ≥ 7. The green histogram represents the implanted synthetic sources, and the gray histogram represents real candidate moving objects. The dashed black line shows the shape of a Gaussian distribution with a mean of zero and a width of one. It is clear that the distribution of ν is very nearly Gaussian. Bottom: distribution of the signal-to-noise ratio of all of the unique candidate trajectories after the tune-up step described in Section 3.4. Real candidates tend to increase in significance, while spurious candidates tend not to. There is a clear boundary at ν = 8.8, beyond which there are probably no false positives.

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