Sterne 2.3 + Spectrum : normalized high-resolution spectra

Spectra calculated using the QUB LTE code Spectrum containing the principal diagnostic lines of H, HeI, HeII, C, N, O and Si used in studies of early-type stars. These files are more compact than the files containing fluxes.

Line 1

LABEL
provides information on the effective temperature, surface gravity, helium abundamces and microturbulent velocity of the model. Compare with line 1 of the model structure.

Line 2

LABEL
normally blank

Line 3

NWAV
The number of wavelength points in the spectrum

Line 4 onwards

WAV(J), FLUX(J), J=1,NWAV
Wavelength (Angstrom), Normalized Flux.

Example

T=15.0 G=2.00 HE=0.001 VT= 5.0 WA= 3970. EW= 5.985
 AB=   5.67
     24753
   3.900000E+03   9.999847E-01
   3.900310E+03   9.999845E-01
   3.900731E+03   9.999843E-01
   3.900760E+03   9.999843E-01
   ...
   4.999280E+03   9.999956E-01
   4.999420E+03   9.999956E-01
   4.999600E+03   9.999956E-01
   4.999830E+03   9.999957E-01
   5.000000E+03   9.999957E-01