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NEOMOD: A New Orbital Distribution Model for Near-Earth Objects

  • Authors: David Nesvorný, Rogerio Deienno, William F. Bottke, Robert Jedicke, Shantanu Naidu, Steven R. Chesley, Paul W. Chodas, Mikael Granvik, David Vokrouhlický, Miroslav Brož, Alessandro Morbidelli, Eric Christensen, Frank C. Shelly, Bryce T. Bolin

David Nesvorný et al 2023 The Astronomical Journal 166 .

  • Provider: AAS Journals

Caption: Figure 4.

The CSS’s mean rate of detection—the number of CSS FOVs in which an NEO with given orbital elements is expected to be detected—is plotted as a function of the absolute magnitude (green line). The average of ﹩{ \mathcal R }(a,e,i,H)﹩, given in Equation (4), was computed over the whole orbital domain. The original bias from Granvik et al. (2018) is shown by open circles. The gray line shows the detection rate when the trailing loss from Zavodny et al. (2008) is not accounted for.

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