Fig. 1.

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Density of spectroscopic and photometric data from training samples as a function of wavelength. A photometric epoch is considered to cover a given wavelength bin if the wavelength is within the FWHM of the filter in the rest-frame. Bin sizes are dictated by the underlying resolution of the SED model. Top two panels show data density with the K21 compilation alone, lower two panels show the K21+ZTF compilation.
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