Table 2: Blöcker track time scales: PN visibility is defined as between $\log T_{\rm eff} = 4.4$ and either a nebular age $t = 10^4~\rm yr$ or a stellar luminosity $\log L = 3.0$, whichever occurs earlier.
Mass [$M_\odot $] $t_{\rm start}$ [yr] $t_{\rm end}$ [yr] $t_{\rm visibility}$ [yr]
0.546 $90 \times 10^3$ - -
0.565 $4 \times 10^3$ $10 \times 10^3$ $6 \times 10^3$
0.605 $1.5 \times 10^3$ $7.4 \times 10^3$ $5.9 \times 10^3$
0.625 660 $3.6 \times 10^3$ $2.9 \times 10^3$
0.696 100 880 780
0.836 100 840 740
0.940 12 90 78

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