Nonuniform cratering of the terrestrial planets

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The orbital distribution of Near-Earth Objects inside Earth's orbit (2012, background): “Le Feuvre and Wieczorek (2008, 2011) found these ratios to be 1.11 and 1.15 respectively.”
How old are young lunar craters (2012, background): “Le Feuvre and Wieczorek [2008] argued that the cratering rate at the lunar poles is 20% less than at the equator. However, Werner and Medvedev [2010] did not find a clear density pattern for craters larger than 5 km.”
Nonuniform cratering of the Moon and a revised crater chronology of the inner Solar System (2011, methodology): “Latitudinal asymmetries are produced by the25 anisotropy of encounter inclinations (Le Feuvre and Wieczorek, 2008), whereas26 7 longitudinal asymmetries result from synchronous rotation since the relative1 encounter velocity, hence impact rate, are maximized at the apex of motion2 (e.g., Morota et…”