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| | [No title] |
 | | Following the prefix "sp" is the lead frequency of the # segment, e. |
 | | For the region 13,500 to 20,000 cm-1, the four # columns of each file contain, first the frequency, second the deduced telluric # spectrum, third the observed photospheric spectrum before correction for # telluric absorption, and fourth the photospheric spectrum corrected for # telluric absorption. |
 | | The required multiplicative factors to # correct the observed frequencies to the laboratory scale are 1.0000013 for # 13,500 to 16,000 cm-1, 0.9999981 for 16,000 to 20,000 cm-1, and 1.0000018 for # 20,000 to 28,000 cm-1. |
| www.astro.wisc.edu /~mab/education/astro920/5010_5263aa.dat (280 words) |
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