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Optical and Infrared Interferometry
Service (and visitor) mode operations by ESO involving the three-beam NIR combiner AMBER on the VLTI are now in their third year, and a large number of observations of calibrators have been accumulated. We present results on the stability of the transfer function, with and without the FINITO fringe tracker, as well as trends and correlations. The reductions were made using publicly available software for AMBER and therefore can be used as a reference for the data quality independent observersdoi:10.1117/12.789060 fatcat:5an3t3odang3bgggytcezxb55u