An overview of the pipeline. Data produced at each of the three detector sites is transfered to a computer at Cascina where triggers are produced by MBTA and sent to GraCEDb for storage. Upon receiving events, GraCEDb alerts the sky localization and data quality check processes to begin and the results are then sent back to GraCEDb. If the triggers are localizable and of acceptable data quality then they are sent out for further processing and possibly followup by an optical telescope. The double stroke connections in the diagram are provided by LVAlert.
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