VizieR Online Data Catalog: Light curve & radial velocity of 4 giants planets (Jordan+, 2022)

HATSouth uses a network of 24 telescopes, each 0.18m in aperture, and 4Kx4K front-side-illuminated CCD cameras. These are attached to a total of 6 fully automated mounts, each with an associated enclosure, which are in turn located at three sites around the Southern Hemisphere. The three sites are Las Campanas Observatory (LCO) in Chile, the site of the HESS gamma-ray observatory in Namibia, and Siding Spring Observatory (SSO) in Australia.

The spectroscopic observations was carried out to confirm and characterize the four transiting planet systems presented here. The facilities used include: Echelle spectrograph on the du Pont 2.54m, 31 WiFeS on the ANU 2.3m, ARCES on the ARC 3.5m, FEROS on the MPG 2.2m, ARCoIRIS on the Blanco 4m, and ESPRESSO on the VLT 8.2m. The du Pont, WiFeS, ARCES, and FEROS observations were obtained only for HATS-74A, while all four systems were observed with ARCoIRIS and ESPRESSO.

(3 data files).