Calibration codes and methods

The data calibration and spectral extraction methods developed in the context of task 1 will be made available first to the consortium, one year after the start of the project. When fully tested and used for task 2, it will be made available to the exoplanet community as a whole via stand-alone code packages and maintained code repositories and as contributed calibration and analysis software to the Spitzer/HST/JWST missions (see WP 6 for dissemination). The theoretical foundations and implementation concepts of the calibrations methods will be fully documented and will be published in peer reviewed journals.