TESS light-curve analysis

Inspect and vet TESS light curves, right in your browser.

Fast Lightcurve Inspector pulls multi-sector TESS photometry from MAST, searches for periods, folds transits, and gives you the vetting tools to tell planets from eclipsing-binary false positives.

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Free · no install · enter any TIC number to begin

Lightcurve Plot · TIC 150428135 QLP
sectors 14, 40, 41 depth ≈ 2,140 ppm P 3.41 d
Pipelines & data
QLPSPOCGSFC ELEANOR-LITETESS-SPOC TESSMASTlightkurveGaia DR3Plotly
Workflow

From a TIC number to a vetted signal.

No downloads, no notebooks. Three steps, all in the browser.

1

Enter a TIC number

Preview which sectors are available across QLP, SPOC, TESS-SPOC and GSFC ELEANOR-LITE, then download only what you need.

2

Plot & search

Stitch multi-sector light curves, run Lomb–Scargle and BLS periodograms, and phase-fold on the best period.

3

Vet the candidate

Check centroids, odd/even depths, secondary eclipses and nearby-star contamination to rule out false positives.

What's inside

The full analysis toolbox.

Everything the app can do — grouped the way you'd actually work through a target.

Fetch & plot light curves

Download multi-sector TESS photometry and stitch it into one interactive Plotly chart. Preview available sectors before you commit.

QLPSPOCGSFC ELEANOR-LITETESS-SPOCMulti-sectorSector Finder

Search for the period

Run Lomb–Scargle and Box Least Squares periodograms. BLS returns the best period, duration and depth to seed the rest of your analysis.

Lomb–ScargleBLSBest period · depth

Fold & measure transits

Phase-fold on any period and epoch to sharpen a repeating signal — and auto-detect the epoch from the deepest transit.

Phase foldAuto epoch

Pixel-level checks

Extract pixel-by-pixel light curves from the target pixel file and view median, in/out-of-transit and difference images to see where the flux drop comes from.

Pixel-by-pixel LCsTPF viewerMedian · In/Out · Diff

Vet false positives

The core of the tool: a battery of checks to separate genuine planets from eclipsing-binary look-alikes — centroid motion in and out of transit, transit-to-transit consistency, secondary eclipses, and light from nearby stars.

Centroid shiftPer-transit evolutionOdd/even depthSecondary eclipseGaia DR3 contaminationΔmag (Kostov+2025)
Free to use

Ready to inspect your first target?

Create a free account and start pulling TESS light curves in seconds. Built for exoplanet vetting, eclipsing binaries and variable-star work.

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