Computer Vision, Neural Radiance Fields, Astronomy, Synthetic Computer Vision, 3d Computer Graphics.
pⁿ(t) = ∫e(t, x)ds Fig 2. 2D Illustration of an emission hot-spot orbiting around a black hole and the resulting 1D image plane projection. As time progresses, t₀ → t₁, the spot is sheared due to the inner radii moving faster than the outer radii. [IMAGE SOURCE: [2]] Hence, by accounting for the