  We report the discovery of HATS-13b and HATS-14b, two hot-Jupiter transiting
planets discovered by the HATSouth survey. The host stars are quite similar to
each other (HATS-13: V = 13.9 mag, M* = 0.96 Msun, R* = 0.89 Rsun, Teff = 5500
K, [Fe/H] = 0.05; HATS-14: V = 13.8 mag, M* = 0.97 Msun, R* = 0.93 Rsun, Teff =
5350 K, [Fe/H] = 0.33) and both the planets orbit around them with a period of
roughly 3 days and a separation of roughly 0.04 au. However, even though they
are irradiated in a similar way, the physical characteristics of the two
planets are very different. HATS-13b, with a mass of Mp = 0.543 MJ and a radius
of Rp = 1.212 RJ, appears as an inflated planet, while HATS-14b, having a mass
of Mp = 1.071 MJ and a radius of Rp = 1.039 RJ, is only slightly larger in
radius than Jupiter.
