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Fig. 6

image

Combined (three nights) residual spectra in the planetary rest frame centered at the 10 830 Å He I line. In the three panels, the solid black line indicates the residual spectra, boxcar-smoothed by 3.7 km s−1 (top), 14.9 km s−1 (middle), and 29.8 km s−1 (bottom). The dotted curves show an artificially injected signal at an S/N of 5, and the solid red curve shows the difference between the injectedand original data. The values are scaled by the standard deviation of the observed residuals so that the y-axis represents the S/N.

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