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Some standard star spectral templates are in form of spiketrum where the absorption lines are avoided to create a smooth continuum-like-spectrum after interpolation. This is not currently handled. Those spiketra have to be identified and the sensitivity curve computation should handle them differently.
The text was updated successfully, but these errors were encountered:
Some standard star spectral templates are in form of spiketrum where the absorption lines are avoided to create a smooth continuum-like-spectrum after interpolation. This is not currently handled. Those spiketra have to be identified and the sensitivity curve computation should handle them differently.
The text was updated successfully, but these errors were encountered: