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P MaNGA: gradients in recent star formation histories as diagnostics for galaxy growth and death

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Figure

Figure 1. P-MaNGA galaxies are plotted as large red or blue symbols on the stellar mass vs
Figure 2. P-MaNGA galaxies are plotted as large red or blue symbols on planes of 4000 Åby solid and dashed lines are solar-metallicity models of continuous star formation histories and star formation bursts calculated using the stellar population synthesis
Figure 3. Example spectra of the P-MaNGA galaxies. The top two rows of panels are for a high-S/N spectrum with S/Nblue line in the lower smaller panel is the difference between the two
Figure 4. Measurements of Dmeasurements obtained by applying our code to the central spaxel of P-MaNGA datacubes and the SDSS spectra, which are compared in red triangles and blackcrosses to the measurements taken from the MPA/JHU database
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