Astronomical Spectroscopy - Physics - University of Cincinnati
Astronomical Spectroscopy - Physics - University of Cincinnati
Astronomical Spectroscopy - Physics - University of Cincinnati
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– 63 –<br />
the only overlap would be with 3000Å from the second order. Given the poor atmospheric<br />
transparency at that wavelength, and the extreme red color <strong>of</strong> such stars, it is safe to assume<br />
that there would be negligible contamination. For the red setting (5000-9000Å) there would<br />
be overlap with second order light