Paper:	Data Flow System for the VLT Interferometer
Volume:	351, Astronomical Data Analysis Software and Systems XV
Page:	271
Authors:	Ballester, P.; Licha, T.; Percheron, I.; Sabet, C.
Abstract:	A milestone on the accuracy of angular measurements is reached with each new instrument on the VLT interferometer: about 10 milliarcsec for MIDI (N Band), 1 milliarcsec for AMBER (JHK bands) and, later, the ultimate goal of 10 microarcsec for the PRIMA imaging and astrometry facility. Extracting the science information from these measurements requires a unified understanding of the data obtained by modeling, homogeneous calibration of large datasets and robust data reduction methods. We describe in this poster the operational tools provided for observation preparation, pipeline processing, and data quality control.

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