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Measurement of the stellar irradiance f - inaoe

Measurement of the stellar irradiance f - inaoe

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Comparison in <strong>the</strong> UV below 2800 Å, where <strong>the</strong>re is an<br />

excellent correlation in <strong>the</strong> wavelengths <strong>of</strong> <strong>the</strong> detailed<br />

spectral features. However, <strong>the</strong> model <strong>of</strong>ten shows an excess<br />

<strong>of</strong> metal-line blanketing by up to several percent.

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