A Real-Time Star Tailing Removal Method Based on Fast Blur Kernel Estimations

Figure 6

The estimation of with noise: (a) sinc curve (when L = 20), (b) processed curve, (c) sinc curve (when L = 5), (d) processed result without weight adjustment, and (e) processed result after weight adjustment.

(a)

(b)

(c)

(d)

(e)