Sterne 2.3 + Spectrum : normalized high-resolution spectraSpectra 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.
provides information on the effective temperature, surface gravity, helium abundamces and microturbulent velocity of the model. Compare with line 1 of the model structure.
The number of wavelength points in the spectrum
Line 4 onwardsWAV(J), FLUX(J), J=1,NWAV
Wavelength (Angstrom), Normalized Flux.
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