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  Automatic observation rendering (AMORE) (Ng, 2002)
Post annotation
1.J/A+A/392/1129/tablea1AMORE results with the test population as specified in Sect. 4.3.1 of the paper (163 rows)
2.J/A+A/392/1129/tablea2Results of running AMORE with one of the astrophysical parameters fixed at its original value (48 rows)
3.J/A+A/392/1129/tablea3AMORE with one of the parameters fixed at one sigma from its original value (90 rows)

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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
   (ALL)Nmodel  (i) [1/162] Model number (;
  (1)pcross  crossover probability (stat.param)
  (1)rcross  multi-point crossover rate (stat.param)
  (1)rbrood  amount of offspring two parents can have (stat.param)
  (1)pcreep  creep mutation rate (stat.param)
  (1)pcorr  correlated mutation rate (stat.param)
   (ALL)fA  Fitness value (stat.param)
  (1)Gen  Generation number (Note 1)   (stat.param)
  (2+3)Param (char) Parameter name (;
  (2+3)logd pc Distance (pos.distance)

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  (2+3)AV mag Extinction (phys.absorption)
  (2+3)logtl [Gyr] Lower age limit (time.age)
  (2+3)logth [Gyr] Upper age limit (time.age)
  (2+3)[Z]l [Sun] Lower metallicity limit (phys.abund.Fe)
  (2+3)[Z]h [Sun] Upper metallicity limit (phys.abund.Fe)
  (2+3)alpha  Slope for the Initial Mass Function power-law (
  (2+3)beta  Index for the Star Formation Rate exponential (
  (3)Offset  Offset in σ units (stat.param)

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