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Table 3

Comparison between observed (P, θ) and those in literature (Schmidt et al. 1992).

Star Nobs ϕ (deg) obs P (%) literature diff obs θ (deg) literature diff
BD+59 389 11 0, 45, 90, 135 6.33 ± 0.03 6.430 ± 0.022 −0.10 97.76 ± 0.12 98.14 ± 0.10 −0.38
HD 154445 7 0, 45, 90, 135 3.76 ± 0.01 3.68 ± 0.07 0.07 88.23 ± 0.28 88.9 ± 0.6 −0.68
HD 19820 1 0 4.77 4.526 ± 0.025 0.24 115.16 114.46 ± 0.16 0.70
HD 204827 2 0,45 5.16 ± 0.04 4.893 ± 0.029 0.27 58.33 ± 0.19 59.10 ± 0.17 −0.77
HD 25443 8 0, 45, 90, 135 4.78 ± 0.07 4.73 ± 0.04 0.05 135.07 ± 0.33 133.65 ± 0.28 1.42

Notes. Number of observations (Nobs) and applied position angles of the FOV (ϕ) are also shown. The observed P and θ are derived from Eqs. (18), (19) for averages and standard errors of Nobs sets of (q, u).

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