We need a list of wavelength bounds to create "chunks" of spectra.
Ideally, these would be well-motivated wavelengths of ~50A each, which hopefully correspond to distinct molecular regions or parameter-sensitive regions.
These chunks would be identical to all stars that we are analyzing, so that we may later link correlations between chunks.
We need a list of wavelength bounds to create "chunks" of spectra.
Ideally, these would be well-motivated wavelengths of ~50A each, which hopefully correspond to distinct molecular regions or parameter-sensitive regions.
These chunks would be identical to all stars that we are analyzing, so that we may later link correlations between chunks.