VizieR Online Data Catalog: RVs and RI-photometry of HATS-37 and HATS-38 (Jordan+, 2020)

The facilities include: the Chilean-Hungarian Automated Telescope (CHAT) 0.7m telescope at Las Campanas Observatory, Chile; 1m telescopes from the Las Cumbres Observatory (LCO) network; the 0.3m Perth Exoplanet Survey Telescope in Australia (PEST); and the Swope 1m telescope at Las Campanas Observatory in Chile. The HATSouth observations of each system are summarized in Table 1.

The spectroscopic observations carried out to confirm and characterize both of the transiting planet systems are summarized in Table 2. The facilities used include Fiber-fed Extended Range Optical Spectrograph (FEROS) on the Max Planck Gesellschaft (MPG) 2.2m, Coralie on the Euler 1.2m, High Accuracy Radial velocity Planet Searcher (HARPS) on the European Southern Observatory (ESO) 3.6m, Wide-Field Spectrograph (WiFeS) on the Australian Nation University (ANU) 2.3m, and Planet Finder Spectrograph (PFS) on the Magellan 6.5m.

(4 data files).