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Table 4

Anderson–Darling (AD) test applied to the histogram densities of the (A,L,G) oscillation spectrum before any pre-whitening process was applied.

A–D test
Star AG AL LG
    
HD50844 (0, 1) (0, 1) (0, 1)
HD174936 (82.7, 1.04 × 10−45) (82,7, 1.04 × 10−45) (0,1)
HD174966 (0, 1) (0, 1) (0, 1)
HD181555 (0, 1) (0, 1) (0, 1)
HD49434 (0, 1) (0, 1) (0, 1)
HD172189 (0, 1) (0, 1) (0, 1)
HD174532 (0, 1) (0, 1) (0, 1)
HD174589 (0, 1) (0, 1) (0, 1)
HD51722 (0, 1) (0, 1) (0, 1)
HD51359 (0, 1) (0, 1) (0, 1)
HD50870 (0, 1) (114,3.45 × 10−63) (114, 3.45 × 10−63)
HD170699 (0, 1) (0, 1) (0, 1)
GSC00144-03031 (0, 1) (0, 1) (0, 1)
HD41641 (0, 1) (112, 1.29 × 10−61) (112, 1.29 × 10−61)
HD48784 (0, 1) (0, 1) (0, 1)

Notes. The pairs AG, AL, and LG represent the compared distributions for the three gap-filling methods considered in this work. The numbers in brackets are the values of the AD test and their corresponding p-values. The null hypothesis is that compared samples arise from a common distribution.

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