The global martian volcanic evolutionary history

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Geologic history of Mars (2010, background): “that the eruption rate was highly episodic (Neukum et al., 2004, 2007; Werner, 2009), an observation supported by the episodic nature of”
Hydrovolcanic tuff rings and cones as indicators for phreatomagmatic explosive eruptions on Mars (2013, background): “[2] Mars was volcanically active throughout most, if not all, of its history [e.g., Werner, 2009; Hauber et al., 2011; Robbins et al., 2011; Xiao et al., 2012], and volcanism played a significant role in the formation of its surface.”
Very recent and wide‐spread basaltic volcanism on Mars (2011, result): “Based on the results shown here [see also Werner, 2009 ] it appears possible that the magmatic activity in Tharsis declined slower than predicted bythese studies,althoughitisdifficult to quantifythevolume of igneous material emplaced in the Amazonian.”
Mars 2020 Mission Overview (2020, background): “Similarly, while both volcanism and impact cratering are ongoing on modern Mars, the rock record shows these processes were far more active geologic agents in the distant past (Frey 2006; Werner 2009; Hauber et al. 2011).”
Mineralogy of the Martian Surface (2014, unknown): “Dust cover in the summit regions of Mars’s highest volcanoes, where the youngest ( 500 Ma) flows lie (Werner 2009), has confounded even the 18 m/pixel scale now enabled by CRISM.”