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| ylabel("rect flux residuals") | ||
| xlabel("Wavelength (Å)") | ||
| savefig("GES_pruned_T_$(Teff)_logg_$(logg).png") | ||
| end No newline at end of file |
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| end | |
| end |
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This script produces a linelist that is slightly over-pruned.
Flux difference at Teff=4000k, logg=3.5, solar abundances:
TODO