

There are 540 different models. For each model there are a number of
files with photometry data, one for each epoch, and there are up to five different epochs
per model, typically two epochs. Each of these files contains photometry data for at least
two pulsation periods.

The identifier for each model is:   'AAAA'l'BBBB'm'CCC'z0.0C'D'_tdrou_u'E'[l20]
where the strings denote:
 'AAAA' is the effective temperature, Teff:  2600, 2800, 3000, 3200 [K]
 'BBBB' is log luminosity:  3.55, 3.70, 3.85, 4.00  [solar luminosities]
 'CCC'  is the stellar mass: 075, 1, 15, 2  [0.75, 1.00, 1.50, 2.00 solar masses]
 'D'    is the carbon excess, log(C-O)+12: 5, 6, 7  [for 8.20, 8.50 and 8.80, respectively]
 'E'    is the piston velocity amplitude:  2, 4, 6  [km/s]
optionally the 'l20' denotes f$_L$ = 2.0, otherwise  f$_L$ = 1.0 [see article]


Each file has 15 columns (written with format: 14f8.3,i8).
The first 10 columns give the synthetic magnitudes in the following filters:
  B, V, R, I, J, H, K, L, L', M 
in the Johnson-Cousins (B,V,R,I; see Bessell 1990, PASP 102, 1181), and
in the Johnson-Glass (J, H, K, L, L', M; see Bessell and Brett 1988, PASP 100, 1134)

Columns 11 - 13 give the 2MASS synthetic magnitudes for J, H and K$_s$, see
Cohen, Wheaton & Megeath 2003, AJ, 126, 1090

Column 14 gives the pulsational phase, with luminosity maxima at 0.0, 1.0 etc

Column 15 gives the snapshot identification number (timestep number).

