VizieR Online Data Catalog: Light curve and radial velocities for 7 host stars (Bakos+, 2021)

We presented the discovery of seven hot Jupiters transiting bright stars. These planets were first identified as transiting planet candidates by the HATNet survey from among some six million stars that have been observed to date since 2004. They were subsequently confirmed and accurately characterized using high-precision time-series photometry from Fred Lawrence Whipple Observatory (FLWO) 1.2 m/KeplerCam, and the NASA Transiting Exoplents Survey Satellite (TESS) mission, and high-resolution spectroscopy, enabling high-precision RVel measurements, carried out with the FLWO 1.5m/TRES (Tillinghast Reflector Echelle Spectrograph), Keck-I/HIRES (High Resolution Echelle Spectrometer), Observatoire de Haute Provence (OHP) 1.93m/SOPHIE, Subaru 8m/HDS, Apache Point Observatory (APO) 3.5m/ARCES, Nordic Optical Telescope (NOT) 2.5m/FIES (fiber-fed echelle Spectrograph), and Las Cumbres Observatory Grand Telescope (LCOGT) 1m/NRES telescopes/instruments. Filters, dates and resolutions can be found in table 1, 2 and 3.

(2 data files).