# Table 1 - Luminosity-specific PN number for Salpeter SSPs(*)
#
# Age  ----------------------------- Metallicity [Z] --------------------------------------
#[Gyr]
#       0.001   0.01   0.017   0.03   IR83      0.001    0.01  0.017   0.03   IR83     W00
#      ---------- \eta = 0.3 --------------    --------------- \eta = 0.5 ----------------- 

  0.1   ...     ...	...    ...  -10.33       ...     ...    ...    ...   -9.71    -8.71
  0.5   ...     ...	...    ...   -8.57       ...     ...    ...    ...   -8.16    -7.22
  1.0   ...     ...	...    ...   -7.98       ...     ...    ...    ...   -7.60    -6.86
  2.0   ...    -7.29   -7.41  -7.41  -7.45       ...    -6.99  -7.02  -7.08  -7.11    -6.60
  3.0   ...    -7.08   -7.15  -7.18  -7.17       ...    -6.70  -6.75  -6.76  -6.85    -6.47
  4.0   ...    -6.90   -6.94  -6.94  -6.98       ...    -6.53  -6.56  -6.55  -6.68    -6.38
  5.0   ...    -6.74   -6.85  -6.88  -6.84       ...    -6.39  -6.40  -6.42  -6.54    -6.32  
  6.0   ...    -6.64   -6.72  -6.73  -6.73       ...    -6.29  -6.30  -6.30  -6.45    -6.30
  8.0  -6.47   -6.46   -6.52  -6.57  -6.56      -6.29  <-6.28 <-6.28 <-6.29  -6.28    -6.27
 10.0  -6.34   -6.31   -6.39  -6.45  -6.44     <-6.27      +      +      +   -6.27    -6.27  
 12.5  -6.29   -6.28   -6.29  -6.30  -6.31         +       +      +      +   -6.27    -6.27
 15.0 <-6.28  <-6.27  <-6.28 <-6.29  -6.27         +       +      +      +  <-6.27   <-6.27
#
# (*) The listed quantity is log \alpha = log N_{PN} - log (L_{SSP}/L_{sun}).
# (+) Planetary nebulae not expected to form for these age/metallicity combinations as M_{PAGB} <= 0.52 M_{sun}.