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starry: Analytic Occultation Light Curves

  • Authors: Rodrigo Luger, Eric Agol, Daniel Foreman-Mackey, David P. Fleming, Jacob Lustig-Yaeger, and Russell Deitrick

2019 The Astronomical Journal 157 64.

  • Provider: AAS Journals

Caption: Figure 5.

Top: phase curves for the first several spherical harmonics with order ﹩m\geqslant 0﹩ rotated about the x-axis (blue) and about the y-axis (orange; Python). Odd harmonics with ﹩l\gt 1﹩ and harmonics with m < 0 are in the phase-curve null space (Cowan et al. 2013). Bottom: occultation light curves for the same set of harmonics. An occultor of radius r = 0.3 transits the body along the ﹩+{\text{}}x﹩ direction at yo = 0.25 (blue) and yo = 0.75 (orange; Python).

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