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Fig. 2

image

Comparison of synchrotron spectra for different CRL models, all normalized to one at 408 MHz. The black solid curve shows the original spectral template used in the Commander analysis, while the cyan solid curve shows the shifted template as described in Planck Collaboration X (2016). In orange is the resulting SED on the plane for synchrotron emission computed using the z10LMPDE CRL model on which the Commander template is based. This curve shows the average curve for the Galactic plane, while the brick red is the average for the pixels on a ring at b = 30°. For these spectra, the effective spectral index is computed. Lastly, the light and dark blue dot-dashed lines show the power law with the effective indices for the z04LMPDS model averaged at the two latitudes.

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