  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 Mjup, and
radii of 1.1 to 1.4 Rjup. 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.
