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We present the discovery of three new transiting giant planets, firstdetected with the WASP telescopes, and establish their planetary nature withfollow up spectroscopy and ground-based photometric lightcurves. WASP-92 is anF7 star, with a moderately inflated planet orbiting with a period of 2.17 days,which has $R_p = 1.461 \pm 0.077 R_{\rm J}$ and $M_p = 0.805 \pm 0.068 M_{\rmJ}$. WASP-93b orbits its F4 host star every 2.73 days and has $R_p = 1.597 \pm0.077 R_{\rm J}$ and $M_p = 1.47 \pm 0.029 M_{\rm J}$. WASP-118b also has a hothost star (F6) and is moderately inflated, where $R_p = 1.440 \pm 0.036 R_{\rmJ}$ and $M_p = 0.513 \pm 0.041 M_{\rm J}$ and the planet has an orbital periodof 4.05 days. They are bright targets (V = 13.18, 10.97 and 11.07 respectively)ideal for further characterisation work, particularly WASP-118b, which is beingobserved by K2 as part of campaign 8. WASP-93b is expected to be tidallymigrating outwards, which is divergent from the tidal behaviour of the majorityof hot Jupiters discovered.

WASP-92b, WASP-93b and WASP-118b: Three new transiting close-in giant planets