The early martian evolution—Constraints from basin formation ages

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The global martian volcanic evolutionary history (2009, background): “Hand in hand with the understanding of the time frame of the decay of the martian magnetic field (Werner, 2008), the thermal evolution and the internal dynamics are more constrained.”
Formation timescales of large Martian valley networks (2011, background): “(2010) that the timing of the impact events (Werner, 2008) coincided with the timing of valley network formation (Fassett and Head, 2008b), hundreds of millions of years span the formation of most of the large impacts (3.”
Large impact crater histories of Mars: The effect of different model crater age techniques (2013, methodology): “densities, while the right panel shows N(16) densities and the martian epoch cut-offs as given in Werner and Tanaka (2011); full bars are where there is agreement between”
Sequence and timing of conditions on early Mars (2011, background): “…consistent with this change have been made on the Moon (Head et al., 2010), Mercury (Fassett et al., manuscript in preparation) and Mars, where Werner (2008) noted that it appears that ‘‘[t]he basin-forming projectile population is most likely different from the general impactor population’’.”