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

<table class="table-group" id="tab1"><tr><td><table class="table"><tr><td class="thead-hr" colspan="2"><hr/></td></tr><tr class="thead"><td class="align_left"> </td><td class="align_center">Time average (s)</td></tr><tr><td class="thead-hr" colspan="2"><hr/></td></tr><tr><td class="align_left">Proposed method</td><td class="align_center">0.0514</td></tr><tr><td class="align_left">Traditional Radon transform method</td><td class="align_center">0.4350</td></tr><tr><td class="align_left">Cepstrum + Radon transform</td><td class="align_center">1.6517</td></tr><tr class="table-tr"><td colspan="2"><hr class="tbody-hr"/></td></tr></table></td></tr></table>

<div>The comparison of computational complexity of different methods.</div>

Mathematical Problems in Engineering

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Table 1

Table 1: A Real-Time Star Tailing Removal Method Based on Fast Blur Kernel Estimations 