We report the discovery of the transiting exoplanets WASP-95b , WASP-96b , WASP-97b , WASP-98b , WASP-99b , WASP-100b and WASP-101b .
All are hot Jupiters with orbital periods in the range 2.1 to 5.7 d , masses of 0.5 to 2.8 M _ { Jup } , and radii of 1.1 to 1.4 R _ { Jup } .
The orbits of all the planets are compatible with zero eccentricity .
WASP-99b shows the shallowest transit yet found by WASP-South , at 0.4 % .

The host stars are of spectral type F2 to G8 .
Five have metallicities of [ Fe/H ] from –0.03 to +0.23 , while WASP-98 has a metallicity of –0.60 , exceptionally low for a star with a transiting exoplanet .
Five of the host stars are brighter than V = 10.8 , which significantly extends the number of bright transiting systems available for follow-up studies .
WASP-95 shows a possible rotational modulation at a period of 20.7 d .

We discuss the completeness of WASP survey techniques by comparing to the HAT project .