Fig. 4.

Measured Hubble constant, before (upper panel) and after (lower panel) correction for the mass along the line of sight as a function of the estimated external convergence. and
are related according to Eq. (16). The dashed black lines show the best linear fit, and the shaded gray envelopes correspond to the 1σ uncertainties. The dotted blue lines represent the relation expected from the theory between
,
and κext.
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