Table 1
Summary of selected TESS FFI light-curve projects, their primary scientific goals, photometric methods, and approximate magnitude limits.
| Project name | Scientific goal(s) | Photometric method | Mag. limit (TESS mag) | References |
|---|---|---|---|---|
| MIT QLP | Transiting exoplanets | Simple aperture Photometry | ≲13.5 | (1) |
| TESS-SPOC | Transiting exoplanets | Simple aperture Photometry | ≲16 | (2) |
| TGLC | Transiting exoplanets | Aperture + PSF Photometry | ≲16 | (3) |
| GSFC-ELEANOR | Transit/stellar variability | Aperture photometry | ≲16 | (4) |
| CDIPS | Transiting exoplanets | Image subtraction | ≲16 | (5) |
| PATHOS | Transiting exoplanets | PSF photometry | ≲16.5 | (6) |
| FGK: V ≤ 13 | ||||
| DIAMANTE | Transiting exoplanets | Image subtraction | M-dwarfs: V ≤ 16, d < 600 pc | (7)(8) |
| TASOC | Asteroseismology | Simple aperture Photometry | ≲15 | (9) |
| T16 | Transit/stellar variability | Image subtraction | ≲16 | (10) |
| TEQUILA | All variable sources | Image subtraction | No imposed limit | (11) |
Notes. (1) Huang et al. (2020); (2) Caldwell et al. (2020); (3) Han & Brandt (2023); (4) Powell et al. (2022); (5) Bouma et al. (2019); (6) Nardiello et al. (2019); (7) Montalto et al. (2020); (8) Montalto (2023); (9) Handberg et al. (2021); (10) Hartman et al. (2025). (11) This work.
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