The PICS Project - I. The impact of metallicity and helium abundance on the bright end of the planetary nebula luminosity function

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Table E.2

PN visibility lifetimes τ_PN,2.5.

t_age	Z
(Gyr)	0.0001	0.001	0.01	0.02	0.04	0.08
0.25	-	-	-	0.00	-	-
0.5	-	0.05	0.38	0.28	0.71	4.17
1.0	-	0.66	3.10	2.28	1.83	4.11
2.0	-	0.81	3.70	3.43	3.35	2.60
4.0	-	1.97	5.43	4.35	4.45	4.28
6.0	-	3.26	7.85	5.84	5.49	5.14
8.0	-	0.01	5.11	4.12	5.95	5.49
10.0	-	-	0.24	1.00	3.93	3.29
12.0	-	-	-	0.39	0.62	3.27
13.0	-	-	-	-	0.41	2.73
τ_PN,2.5 in units of 10³ yr

Notes. The PN visibility lifetimes τ_PN,2.5 are given in units of 10³ yr and are determined from the PNe with M(5007) < -2.0 resulting from the SSPs. Each row corresponds to the given age t_age and each column to the given metallicity Z.

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