Three-dimensional interferometric, spectrometric, and planetary views of Procyon

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Table 3

Best-fit angular diameters, in mas, for RHD simulation with method (1) (θ_Method1) and method (2) (θ_Method2) described in Sect. 3.1; and for the uniform disk.

Filter	θ_Method1	θ_Method2	θ_UD

Mark 500 nm	5.313 ± 0.03	5.324 ± 0.03	5.012 ± 0.03
Mark 800 nm	5.375 ± 0.06	5.370 ± 0.06	5.208 ± 0.06
Vinci	5.382^a ± 0.03	5.397^a ± 0.03	5.326 ± 0.03

Notes. The error is one σ with respect to the average value.

^(a)

Since the resulting diameters are very similar, we adopted an average angular diameter of 5.390 for all the calculations in the article.

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