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Spectral atlas : ウィキペディア英語版 | Spectral atlas
In astronomy, a spectral atlas is a collection of spectra of one or more objects, intended as a reference work for comparison with spectra of other objects. Several different types of collections are titled spectral atlases: those intended spectral classification, for key reference or as a collection of spectras of a general type of object. In any spectral atlas, generally all the spectra have been taken with the same equipment, or with very similar instruments at different locations, to provide data as uniform as possible in its spectral resolution, wavelength coverage, noise characteristics, etc. ==Types==
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