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We present the discovery of two new hot Jupiters identified from the WASPsurvey, WASP-186b and WASP-187b (TOI-1494.01 and TOI-1493.01). Their planetarynature was established from SOPHIE spectroscopic observations, and additionalphotometry was obtained from TESS. Stellar parameters for the host stars arederived from spectral line, IRFM, and isochrone placement analyses. Theseparameters are combined with the photometric and radial velocity data in anMCMC method to determine the planetary properties. WASP-186b is a massiveJupiter (4.22 +/- 0.18 M_J, 1.11 +/-0.03 R_J) orbiting a mid-F star on a 5.03day eccentric (e=0.327 +/- 0.008) orbit. WASP-187b is a low density (0.80 +/-0.09 M_J, 1.64 +/- 0.05 R_J) planet in a 5.15 day circular orbit around aslightly evolved early F-type star.

WASP-186 and WASP-187: two hot Jupiters discovered by SuperWASP and SOPHIE with additional observations by TESS