The halo of M 105 and its group environment as traced by planetary nebula populations - I. Wide-field photometric survey of planetary nebulae in the Leo I group

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Fig. B.1.

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Posterior probability distribution of the parameters μ_const and α_outer/α_inner of the two-component model with constant outer SB profile. The red lines denote the best-fit parameters determined in Sect. 4.2 (see Table 2), and the dashed lines show the 16%, 50%, and 84% levels.

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