VizieR Online Data Catalog: WASP 95-101 transits (Hellier+, 2014)

The observational and analysis techniques used here are the same as in recent WASP discovery papers (e.g. Hellier et al., 2012MNRAS.426..739H, Cat. J/MNRAS/426/739).

In outline, WASP-South surveys the visible sky each clear night using an array of 200 mm f/1.8 lenses and a cadence of ~10-min. Transit searching of accumulated light curves leads to candidates that are passed to TRAPPIST (a robotic 0.6-m photometric telescope, which can resolve blends and check that the candidate transits are planet-like), and to the 1.2-m Euler/CORALIE spectrograph [for radial-velocity (RV) observations]. About 1 in 12 candidates turns out to be a planet. Higher quality transit light curves are then obtained with TRAPPIST and with EulerCAM (Lendl et al., 2012A&A...544A..72L, Cat. J/A+A/544/A72).

(2 data files).