Abstract: The high-contrast imager SPHERE at the Very Large Telescope combines extreme adaptive optics and coronagraphy to directly image exoplanets in the near-infrared. The vlt-sphere package enables easy reduction of the data coming from IRDIS and IFS, the two near-infrared subsystems of SPHERE. The package relies on the official ESO pipeline (ascl:1402.010), which must be installed separately.
Credit: Vigan, Arthur
Preferred citation method: https://ui.adsabs.harvard.edu/abs/2020ascl.soft09002V; please see additional citation information here: https://github.com/avigan/SPHERE#credits