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Table 4

Relative radial velocities and bisector spans of HAT-P-42 and HAT-P-43.

Object BJDa RVb σ RV c BISd Phase
−2   455   000 m   s-1 m   s-1 m   s-1

HAT-P-42 889.03539 −47.4 28.4 ···  0.322
900.05380 159.1 33.8 ···  0.696
901.01864 27.1 32.4 ···  0.904
902.02682 −105.1 34.6 ···  0.121
902.71983 −112.1 13.0 −43.0 0.270
902.93220 −75.4 25.4 ···  0.316
903.67805 8.9 31.0 −27.0 0.477
904.03850 −14.2 25.4 ···  0.554
904.66696 97.9 38.0 5.0 0.690
905.02718 75.3 29.9 ···  0.767
906.60475 −46.1 44.0 8.0 0.107
907.02711 −33.4 25.9 ···  0.198
908.63608 71.9 69.0 −35.0 0.545
939.89586 −166.5 33.4 ···  0.279

HAT-P-43 901.68768 −85.8 15.0 −36.0 0.289
902.67245 40.3 15.0 −77.0 0.585
903.62875 42.3 31.0 12.0 0.872
904.62601 −94.8 27.0 −18.0 0.171
906.57509 111.3 28.0 −26.0 0.756
908.60322 −28.8 31.0 35.0 0.364

Notes. Observations without a BIS value were obtained with the TRES instrument, observations with a BIS value were obtained with SOPHIE.

(a)

Barycentric Julian Date calculated directly from UTC, without correction for leap seconds.

(b)

A zero-level γ velocity, fitted independently for each instrument, has been subtracted from these measurements. For reference, for HAT-P-42, the SOPHIE γ velocity from the fit was 20.561 ± 0.014 km   s-1, which is an estimate of the true recession velocity of the center of mass of the system. For TRES the value is 0.014 ± 0.015 km   s-1. As an artifact of the reduction procedure the TRES RVs were measured relative to an arbitrary zero-point, the fitted γ velocity in this case has no physical meaning. For HAT-P-43, the SOPHIE γ velocity from the fit was −5.082 ± 0.009 km   s-1.

(c)

Internal errors excluding any component of astrophysical jitter.

(d)

We use the relation σBIS = 2σRV to estimate the BIS uncertainties.

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