Fig. B.2
Histogram of determined rms noise (given in antenna temperature values) for all spectra in the GRS. Theinset shows the same distribution on a logarithmic scale. The red line in the inset indicates masked out spectra with high noise values. The grey-shaded area marks the IQR, ranging from about 0.1− 0.16 K. The bin width is 0.005 K.
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