Project to prepare and enable the NOvA Experiment to meet their Monte Carlo and production needs for the first physics analysis results from the Far Detector.
The project focuses on the development of key infrastructure in the NOvA software suite that will allow the Monte Carlo generation, key stages of production and reconstruction to run on both FermiGrid resources and resources at offsite institutions. This project includes the deployment of a CVMFS infrastructure for the distribution of NOvA code and for the dissemination of the calibration and analysis template files. It also includes the modification of existing software to support running under a CVMFS distribution structure and the development (where necessary) of new software infrastructure.
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