The first set of tutorials cover the basics of using Lightkurve. This includes getting to grips with the file types and how to load and work with data from the Kepler, K2, and TESS missions.
01-target-pixel-files.ipynb 01-what-are-lightcurves.ipynb 01-lightcurve-files.ipynb 01-using-the-periodogram-class.ipynb
In the second section we cover some data analysis tasks that astronomers might commonly want to do with time series data.
02-recover-a-planet.ipynb 02-how-to-recover-the-first-tess-candidate.ipynb 02-how-to-use-lightkurve-for-asteroseismology.ipynb 02-how-to-make-a-supernova-lightcurve.ipynb
The third section focuses on the various ways in which light curves can be extract from the pixel data.
03-making-custom-apertures.ipynb 03-how-to-use-prf-photometry.ipynb 03-cutting-out-tpfs-from-tess-ffis.ipynb 03-making-fits-files.ipynb 03-appending-lightcurves.ipynb
The final section focuses on the removal of instrument noise.
04-interact-with-lightcurves-and-tpf.ipynb 04-removing-cbvs.ipynb 04-how-to-detrend.ipynb 04-replicate-vanderburg-2014-k2sff.ipynb 04-replicate-vanderburg-2014-lightkurve.ipynb 04-identify-rolling-band.ipynb