WASP-South transiting exoplanets: WASP-130b, WASP-131b, WASP-132b,   WASP-139b, WASP-140b, WASP-141b & WASP-142b
  We describe seven exoplanets transiting stars of brightness V = 10.1 to 12.4. WASP-130b is a "warm Jupiter" having an orbital period of 11.6 d around a metal-rich G6 star. Its mass and radius (1.23 +/- 0.04 Mjup; 0.89 +/- 0.03 Rjup) support the trend that warm Jupiters have smaller radii than hot Jupiters. WASP-131b is a bloated Saturn-mass planet (0.27 Mjup; 1.22 Rjup). Its large scale height and bright (V = 10.1) host star make it a good target for atmospheric characterisation. WASP-132b (0.41 Mjup; 0.87 Rjup) is among the least irradiated and coolest of WASP planets, having a 7.1-d orbit around a K4 star. WASP-139b is a "super-Neptune" akin to HATS-7b and HATS-8b, being the lowest-mass planet yet found by WASP (0.12 Mjup; 0.80 Rjup). The metal-rich K0 host star appears to be anomalously dense, akin to HAT-P-11. WASP-140b is a 2.4-Mjup planet in an eccentric (e = 0.047 +/- 0.004) 2.2-d orbit. The planet's radius is large (1.4 Rjup), but uncertain owing to the grazing transit (b = 0.93). The 10.4-day rotation period of the K0 host star suggests a young age, and the timescale for tidal circularisation is likely to be the lowest of all known eccentric hot Jupiters. WASP-141b (2.7 Mjup, 1.2 Rjup, P = 3.3 d) and WASP-142b (0.84 Mjup, 1.53 Rjup, P = 2.1 d) are typical hot Jupiters orbiting metal-rich F stars. We show that the period distribution within the hot-Jupiter bulge does not depend on the metallicity of the host star. 
Coel Hellier, D.R. Anderson, A. Collier Cameron, L. Delrez, M. Gillon,   E. Jehin, M. Lendl, P.F.L. Maxted, M. Neveu-VanMall...
astro-ph.EP