Abstract
Based on long-term observations of the absolute energy distribution in stellar spectra (starting in 1975), and from a survey of the literature, 14 stars of early spectral type (B7 III–A7 V) were selected. The constancy of their brightness is beyond any doubt now. These stars, with visual magnitudes 0.0 to 4.8, can be recommended as spectrophotometric standards for the spectral region 310–750 nm.
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Terez, E.I. List of stars recommended as spectrophotometric standards. Sol Phys 152, 87–90 (1994). https://doi.org/10.1007/BF01473188
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DOI: https://doi.org/10.1007/BF01473188