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Table 2.

Orbital phases of the centroids of BP1, BP2 and the IP, , and the corresponding 3σ widths, , as a function of MJD, estimated via Gaussian fits to the distribution of S/N of the observed profiles (see Fig. B.1).

MJD ⟨MJD⟩
53000–53100 53018.1 0.573(1) 0.154(9) 0.782(3) 0.12(2)
53100–53200 53144.7 0.579(1) 0.140(6) 0.779(3) 0.14(2) 0.051(2) 0.07(1)
53200–53300 53231.8 0.5753(9) 0.128(6) 0.792(2) 0.11(1) 0.03(1) 0.25(7)
53300–53400 53373.1 0.5786(4) 0.109(3) 0.795(1) 0.106(7) 0.02(1) 0.25(7)
53400–53500 53464.5 0.5781(4) 0.097(2) 0.7956(8) 0.109(5) 0.04(1) 0.22(4)
53500–53600 53528.0 0.5805(2) 0.104(1) 0.7988(5) 0.119(3) 0.034(4) 0.22(2)
53600–53700 53646.2 0.5817(4) 0.110(2) 0.7999(7) 0.115(4) 0.04(1) 0.28(6)
53700–53800 53701.9 0.5813(2) 0.107(1) 0.8015(4) 0.115(2) 0.040(7) 0.23(4)
53800–53900 53849.6 0.5832(3) 0.098(2) 0.8054(3) 0.107(2) 0.04(1) 0.31(7)
53900–54000 53944.4 0.589(1) 0.110(7) 0.805(2) 0.131(9)
54000–54100 54053.9 0.5899(4) 0.097(2) 0.8069(4) 0.112(3)
54100–54200 54186.3 0.5936(4) 0.095(3) 0.8072(5) 0.106(3)
54300–54400 54373.6 0.600(5) 0.15(3) 0.808(1) 0.079(8)
54400–54500 54433.3 0.6027(8) 0.095(5) 0.8088(7) 0.096(4)

Notes. All orbital phases are shown as a fraction of the orbit, measured from the ascending node. The 1σ errors in parentheses correspond to the last significant digit. The second column shows the mean MJD, weighted by the number of observations.

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