VizieR Online Data Catalog: LCs and RVs of 5 exoplanets discovered by TESS (Rodriguez+, 2021)

The initial detection of the new planets came from data collected by the Transiting Exoplanet Survey Satelliyte (TESS) mission. TESS images the sky with a 24x96° field of view and observes the same stars for about a month before moving on to observe a different region.

We obtained photometric follow-up observations on all five systems from the TESS Follow-up Observing Program Working Group subgroup 1 (SG1) for seeing-limited photometry. Specifically, the follow-up comes from the Las Cumbres Observatory (LCO) telescope network, Whitin Observatory at Wellesley College, KeplerCam on the 1.2m telescope at Fred Lawrence Whipple Observatory (FLWO), Brierfield Observatory, PEST Observatory, C. R. Chambliss Astronomical Observatory (CRCAO) at Kutztown University, Adams Observatory at Austin College, and Suto Observatory. To schedule the photometric transit follow-up observations, we used the TAPIR software package.

To confirm targets from TESS in the Northern hemisphere, we observed TOI-628, TOI-1333, TOI-1478, and TOI-1601 with the Tillinghast Reflector Echelle Spectrograph (TRES) on the 1.5m Tillinghast Reflector. The telescope is located at the Fred L.Whipple Observatory on Mt. Hopkins, AZ, and the spectrograph has a resolving power of R=44000. We obtained a series of spectroscopic observations with the 1.5m SMARTS/CHIRON facility for TOI-640 and TOI-1478. Using the FEROS spectrograph mounted on the 2.2m MPG telescope at La Silla observatory in Chile, we obtained eight observations of TOI-1478. FEROS has R=48000 TOI-1478 was observed with the CORALIE high-resolution spectrograph (R=60000) on the Swiss 1.2m Euler telescope at La Silla Observatories, Chile. TOI-628 was monitored by Minerva-Australis (R=80000) using two or three telescopes.

(3 data files).