Transit-vetting is a small webapp that allows the use of TESS-Centroid_vetting to analyze a single transit in a TESS lightcurve.
The user should provide a TIC and a sector number (any sector observed by TESS for the target).
The corresponding lightcurve is displayed and the user can interact with it (thx to Plotly), zooming/panning/selecting any transit that will be analyzed.
The transit being selected, TESS-Centroid-vetting is called and displayed, showing the PRF Centroid of the difference image, and the distance to the nearest stars to it.
You can access the webapp locally in a Python environmente with the command:
streamlit run transit-vetting.py
and the app will open in the default browser.
This webapp is also currently hosted in Streamlit Cloud. You can access it at
If more than one author is available for the sector, the displayed lightcurve, in availability order, is: SPOC (2 min) -> TESS-SPOC -> QLP -> ELEANOR.
If the sector is only available in FFI data, an FFI cutout is made to get a targetpixelfile that, after background subtraction, is used to generate the lightcurve
- numpy
- pandas
- lightkurve
- plotly
- tesscentroidvetting >= 1.3.4
- streamlit