Fig. 12
Correlations in ecliptic coordinates (five-parameter solutions, G = 13–16). Left: mediancorrelation coefficient between errors in ecliptic longitude (λ) and latitude (β). Right: same for the proper motion components (μλ*, μβ ). Contrary to other sky maps in the paper, these two use a projection in ecliptic coordinates with λ = β = 0 in the centre.
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