The Kvis program process raw data (Level 0) from the Keck Interferometer into internally calibrated visibilities (Level 1 data). It is the first program in the visibility data processing pipeline and is generally followed by applying external calibrations using wbCalib or nbCalib. Details of how Kvis processes the data are contained in the users guide.
In addition to the processing program, the Kvis distribution includes plotting and pipeline scripts. The plotting script(KvisPlot) is described in the users manual and links to the other scripts are given below.
updated 8/20/02 R. Akeson
The NASA Exoplanet Science Institute is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program.
