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We present observations of the Rossiter–McLaughlin effect for the transiting exoplanets WASP‐1b, WASP‐24b, WASP‐38b and HAT‐P‐8b, and deduce the orientations of the planetary orbits with respect to the host stars’ rotation axes. The planets WASP‐24b, WASP‐38b and HAT‐P‐8b appear to move in prograde orbits and be well aligned, having sky‐projected spin‐orbit angles consistent with zero: λ=−47 ± 40,...
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