The TESS Objects of Interest Catalog from the TESS Prime Mission
arXiv:2103.12538 · doi:10.3847/1538-4365/abefe1
Abstract
We present 2,241 exoplanet candidates identified with data from the Transiting Exoplanet Survey Satellite (TESS) during its two-year prime mission. We list these candidates in the TESS Objects of Interest (TOI) Catalog, which includes both new planet candidates found by TESS and previously-known planets recovered by TESS observations. We describe the process used to identify TOIs and investigate the characteristics of the new planet candidates, and discuss some notable TESS planet discoveries. The TOI Catalog includes an unprecedented number of small planet candidates around nearby bright stars, which are well-suited for detailed follow-up observations. The TESS data products for the Prime Mission (Sectors 1-26), including the TOI Catalog, light curves, full-frame images, and target pixel files, are publicly available on the Mikulski Archive for Space Telescopes.
39 pages, 16 figures. The Prime Mission TOI Catalog is included in the ancillary data as a CSV. For the most up-to-date catalog, refer to https://tess.mit.edu/toi-releases/
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- Quantifying the Effect of Short-timescale Stellar Activity Upon Transit Detection in M Dwarfs
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- Three Hot Jupiters transiting K-dwarfs with a significant heavy element mass
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- Discovery of a transiting hot water-world candidate orbiting Ross 176 with TESS and CARMENES
- The GAPS programme at TNG LXXI. A sub-Neptune suitable for atmospheric characterization in a multiplanet and mutually inclined system orbiting the bright K dwarf TOI-5789 (HIP 99452)
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- A distant brown dwarf coplanar to a warm Jupiter and a hot super-Earth
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- Two New roAp Stars Discovered with TESS
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- Orbital alignment of HD 332231 b
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- A large sub-Neptune transiting the thick-disk M4V TOI-2406
- Multicolour Validation of Two Temperate Mini-Neptunes Around M-dwarf Habitable Zones
- Generating Stellar Obliquity in Systems with Broken Protoplanetary Disks
- A Uniform Search for Nearby Planetary Companions to Hot Jupiters in TESS Data Reveals Hot Jupiters are Still Lonely
- SpinSpotter: An Automated Algorithm for Identifying Stellar Rotation Periods With Autocorrelation Analysis
- Revisiting BD-06 1339b: A Likely False Positive Caused by Stellar Activity
- Validating the Orbital Periods of the Coolest TESS Exoplanet Candidates
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