VizieR Online Data Catalog: Rot. distributions from TESS-APOGEE-Kepler-Gaia (Avallone+, 2022)
Abstract
We use Cycle 1 data from the Transiting Exoplanet Survey Satellite (TESS) southern continuous viewing zone (SCVZ) and spectroscopic parameters from an APOGEE External Program through Carnegie Observatories.
APOGEE data are collected with the 2.5m Sloan Digital Sky Survey (SDSS) telescope at Apache Point Observatory and with the 2.5m du Pont telescope at Las Campanas Observatory using near-twin H-band spectrographs as part of the fourth campaign of SDSS (SDSS-IV). APOGEE DR16 plus includes observations up to 2020 March (MJD=58932), and APOGEE DR16 (III/284) includes observations up to August 2018 (MJD=58358). We augment our TESS-APOGEE SCVZ sample with stars observed by APOGEE and the Kepler Space Telescope. We finally use stellar parallaxes from Gaia data release 2 (I/345), K-band magnitudes from 2MASS (II/246), and Teff and [Fe/H] from APOGEE to improve our estimates of the radii of stars in our final sample. See Section 2. (2 data files).- Publication:
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VizieR Online Data Catalog
- Pub Date:
- March 2024
- Bibcode:
- 2024yCat..19300007A
- Keywords:
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- Rotational velocities;
- Abundances;
- Stars: diameters;
- Stars: masses;
- Photometry;
- Optical;
- Binaries: spectroscopic;
- Infrared sources