Last Updated：2025/11/22
Sentence
星の光度を求める際、天文学者はしばしば可視域外で放射される光を考慮して、その星の全光度等級と可視等級の差（全光度補正）を適用します。
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When determining a star's luminosity, astronomers often apply a bolometric correction to account for light emitted outside the visible range.
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When determining a star's luminosity, astronomers often apply a bolometric correction to account for light emitted outside the visible range.
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bolometric correction
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