Continuous lines represent the planetary radial velocity during the transit for different values of the eccentricity (e) and the longitude of periastron (ω). In this figure we assumed ms = 1 M⊙, mp = 1 Mjup, i = 90°, P = 3 days. The dotted lines indicate the mid-transit point and the systemic velocity. The box in the lower right corner is a magnified view close to the mid-transit point.
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