VizieR Online Data Catalog: Photometry & RVs of 4 dwarfs hosting giant planets (Hartman+, 2020)

All four systems were observed by the NASA TESS mission as summarized in Table1.

HATS-72 was observed by WASP-South over the period 2006-May to 2012-June, accumulating 24200 data points. WASP-South is an array of eight cameras combining 200mm f/1.8lenses with 2kx2k CCDs and observing with a broad, 400-700nm bandpass. It observed visible fields with a typical cadence of 15minutes on each clear night. After identification of a candidate 7.33day transit periodicity, HATS-72 was placed on the WASP-South follow-up program in 2013-January. This led to nine RVs being observed with the Euler/CORALIE spectrograph over 2013-2018, and the observation in 2018-July of a transit with TRAPPIST-South, using an I+z filter.

The spectroscopic observations carried out to confirm and characterize the four transiting planet systems presented here are summarized in Table3. The facilities are: WiFeS on the Australian National university (ANU) 2.3m, Planet Finder Spectrograph (PFS) on the Magellan 6.5m, Fiber-fed Extended Range Optical Spectrograph (FEROS) on the Max Planck Society (MPG) 2.2m, High Accuracy Radial velocity Planet Searcher (HARPS) on the European Southern Observatory (ESO) 3.6m, Coralie on the Euler 1.2m, and Echelle SPectrograph for Rocky Exoplanets and Stable Spectroscopic Observations (ESPRESSO) on the Very Large Telescope (VLT) 8.2m.

(5 data files).