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- Full Frame Images (FFI, ffi.fits): These files contain the long cadence time series of the entire field of view, both an uncalibrated and calibrated version are available.
- Target Pixel Files (TPF, .tp.fits): These files contain a time series of the raw and calibrated pixels downloaded at the 2-minute cadence.
- Light Curve Files (LCF, .lc.fits): These files contain the simple aperture photometry flux time series derived from the calibrated short-cadence pixels. It also contains a conditioned light curve that attempts to remove all signals except for astrophysical ones by co-trending against basis vectors derived from all stars observed in short cadence on the same camera.
Target Catalogs
Tess provides several catalogs of target stars in order to choose which stars will be observed at a rapid cadence.
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- DV Time Series Files (.dvt.fits): These files contain the sector-stitched, detrended and whitened light curves searched by the TESS Pipeline. All TCEs found on a star in one search are contained in the same file.
- DV Reports (.dvr.pdf): These pdf files contain plots and statistics for each TCE. For example, the reports contain plots of folded light curves and in- and out-of transit difference images.
- DV One-Page Summary (.dvs.pdf): This one page summary contains a quick overview of each TCE and much of the most important information about the TCE to determine if the signal is likely caused by a transit or shows evidence of being caused by an eclipsing binary or instrumental noise. Each TCE gets its own file, so if multiple TCEs are found on the same target star, there will be multiple pdf files.
Results Catalogs
TESS produces several catalogs of possibly transit-like, periodic signals in the TESS data. As the diagram above indicates, these catalogs contain overlapping populations each with different levels of signal vetting. The Threshold Crossing Events (TCE) found in the short cadence time series by the SPOC pipeline (as well as signals found by searching light curves created from the TESS FFIs) are turned into TESS Objects of Interest (TOI) once the signal is vetted and determined to be sufficiently consistent with a transit or eclipse. The TOI list contains both planet candidates and false positives. The false positives are those with evidence of being an eclipsing binary. Once follow-up measurements reveal the mass of the transiting object, or remove all doubt that the signal could be caused by an eclipsing binary, the planet is considered confirmed.
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