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There are 799 tables. Each table has 2 columns. The number of lines is different
for each table. Column 1 is time in years, column 2 is the synthesized galaxy
property as discussed in the paper. The names of all files are LH95.xxxxx,
standing for Leitherer and Heckman 1995. Each table contains the numbers used
for the generation of the curves in the 71 figures of the paper. Since there
is more than 1 curve in each figure, there are more than 71 tables.

The filename uniquely identifies the corresponding figure. For instance,
LH95.F1_xxxx has the models of Figure 1, and LH95.F71_xxxx refers to Figure 71.
Figures 1 through 58 and 66 through 71 are identical in their structure. Each
of these figures has 12 curves (3 in each of the 4 sub-figures). The curves
are for 4 different metallicities and 3 different IMF parameters. 
Nomenclature: 
M10 - metallicity of Minus 1.0 (i.e. 0.1 solar)
M06                  Minus 0.6 (i.e. 0.25 solar)
P00                  Plus  0.0 (i.e. solar)
P03                  Plus  0.3 (i.e. 2 solar)
235 - IMF slope of 2.35
330                3.30
30    cut-off mass of 30

Example:  LH95.F10_M06_330 corresponds to Figure 10, metallicity 0.25 solar,
and IMF slope of 3.3


Figures 59, 60, and 61 contain 5 curves each. Each curve is based on a
different burst duration. 
Nomenclature:
T00 - duration of 0 Myr
T01               1 Myr
T03               3 Myr
T10              10 Myr
T50              50 Myr

Example:  LH95.F59_T10 is the 10 Myr model in Figure 59.


Fiugres 62 through 65 have 4 curves each. They show the synthesized quantities
with and without nebular emission for an instantaneous and continuous burst.
Nomenclature:
NEB     - nebular continuum included
NONEB     nebular continuum not included
BURST     instantaneous burst
CONT      continuous star formation

Example:  LH95.F63_NONEB_CONT is the model without nebular continuum in a
continuous burst in Figure 63.