  We present the discovery and characterisation of the exoplanets WASP-113b and
WASP-114b by the WASP survey, {\it SOPHIE} and {\it CORALIE}. The planetary
nature of the systems was established by performing follow-up photometric and
spectroscopic observations. The follow-up data were combined with the
WASP-photometry and analysed with an MCMC code to obtain system parameters. The
host stars WASP-113 and WASP-114 are very similar. They are both early G-type
stars with an effective temperature of $\sim 5900\,$K, [Fe/H]$\sim 0.12$ and
$T_{\rm eff}$ $\sim 4.1$dex. However, WASP-113 is older than WASP-114. Although
the planetary companions have similar radii, WASP-114b is almost 4 times
heavier than WASP-113b. WASP-113b has a mass of $0.48\,$ $\mathrm{M}_{\rm Jup}$
and an orbital period of $\sim 4.5\,$days; WASP-114b has a mass of $1.77\,$
$\mathrm{M}_{\rm Jup}$ and an orbital period of $\sim 1.5\,$days. Both planets
have inflated radii, in particular WASP-113 with a radius anomaly of
$\Re=0.35$. The high scale height of WASP-113b ($\sim 950$ km ) makes it a good
target for follow-up atmospheric observations.
