  We present the discovery of two new hot Jupiters identified from the WASP
survey, WASP-186b and WASP-187b (TOI-1494.01 and TOI-1493.01). Their planetary
nature was established from SOPHIE spectroscopic observations, and additional
photometry was obtained from TESS. Stellar parameters for the host stars are
derived from spectral line, IRFM, and isochrone placement analyses. These
parameters are combined with the photometric and radial velocity data in an
MCMC method to determine the planetary properties. WASP-186b is a massive
Jupiter (4.22 +/- 0.18 M_J, 1.11 +/-0.03 R_J) orbiting a mid-F star on a 5.03
day 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 a
slightly evolved early F-type star.

Earth and Planetary Astrophysics