📺 denotes a narrated screencast is available on the Kepler/K2 Guest Observer Office YouTube Channel.
- What are TargetPixelFile objects? 📺
- What are LightCurve objects? 📺
- What are LightCurveFile objects? 📺
- What is the Periodogram class? 📺
- How to recover a known planet in Kepler data?
- How to recover the first TESS planet candidate with Lightkurve?
- How to use lightkurve for asteroseismology
- How to make a supernova lightcurve?
- How to perform aperture photometry with custom apertures?
- How to perform PRF photometry?
- How to cut out Target Pixel Files from Kepler Superstamps or TESS FFIs?
- How to save a LightCurve in FITS format?
- How to combine lightcurves from different Kepler quarters
- How do you use river plots?
- Interactively inspecting Target Pixel Files and Lightcurves 📺
- How to remove common systematics using basis vectors (CBVs)
- How to remove K2 motion systematics with SFF?
- How does the SFF method work? 📺
- Replicating Vanderburg & Johnson 2014 using lightkurve 📺
- How to identify time-variable background noise (“rolling bands”)?