Sterne 2.3 Model Atmosphere Fluxes
These (q) files contain the Sterne model atmosphere fluxes formatted for input to the spectral analysis software DIPSO. The format is sometimes known as "SPECTRUM format 2" and is easily read into other analysis software. It is defined as follows:Line 1
LABEL
provides information on the effective temperature, surface gravity and surface composition of model. Compare with line 1 of the model structure.Line 2
LABEL
normally blankLine 3
NWAV
The number of wavelength points in the spectrumLine 4 onwards
WAV(J), FLUX(J), J=1,NWAV
Wavelength (Angstrom), Flux (erg/cm^2/s/A).Example
STERNE: Teff=14000. log g=2.0 H=0.00 He=0.99 CN=0.01031 342 229.0 0.59488E-10 234.0 0.18072E-09 243.0 0.11816E-08 252.0 0.68211E-08 256.0 0.13932E-07 260.0 0.31810E-07 266.0 0.87901E-07 275.0 0.37018E-06 .... 27000.0 0.14231E+06 40000.0 0.30978E+05 50000.0 0.12986E+05 65000.0 0.46425E+04 100000.0 0.85079E+03 200000.0 0.54588E+02