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The origins of post starburst galaxies at z < 0 05

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Figure

Table 1. Balmer-strong galaxy counts in the final samples and a summary of the sample selection criteria (see Section 2.1 for details).Cuts that were omitted during selection of particular samples are marked as not applicable (N/A) - note this does not mean
Figure 2. The distribution of various spectral indicators for all galaxies in the parent samples (grayscale) with the final Balmer-stronggalaxies (see Section 2.2.1 for selection details) overplotted in orange (qPSB), yellow (agnPSB), dark blue (ePSB) and p
Figure 3. Top panel: the stacked SED of the different galaxy samples, normalised at 8000lines that of [NII]6583are zoomed-in on in the bottom panel and in Figure 4
Figure 4. Portions of the stacked SED presented in the top panel of Figure 3 containing particular regions of interest
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