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Table 10
Influence of wavelength grid correction by a Chebyshev polynomial of order wlc_n on the telluric absorption correction of the spectrum displayed in Fig. 2 for the fixed best-fit line profile (relres_box = 0.560 and res_gauss = 1.671) as derived from the standard test run.
| wlc_n | Rel. | FWHM | PWV | Ioff | Ires |
| rms | [pixels] | [mm] | |||
|
|
|||||
| 0 | 0.054 | 3.75 | 1.47 | −0.007 | 0.235 |
| 1 | 0.031 | 3.75 | 1.44 | −0.028 | 0.195 |
| 3 | 0.040 | 3.75 | 1.39 | −0.042 | 0.262 |
| 5 | 0.031 | 3.75 | 1.42 | −0.021 | 0.343 |
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