期刊
ASTRONOMY & ASTROPHYSICS
卷 425, 期 3, 页码 1161-1174出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20034562
关键词
techniques : interferometric; methods : data analysis; instrumentation : interferometers
The interferometric data processing methods that we describe in this paper use a number of innovative techniques. In particular, the implementation of the wavelet transform allows us to obtain a good immunity of the fringe processing to false detections and large amplitude perturbations by the atmospheric piston effect, through a careful, automated selection of the interferograms. To demonstrate the data reduction procedure, we describe the processing and calibration of a sample of stellar data from the VINCI beam combiner. Starting from the raw data, we derive the angular diameter of the dwarf star a Cen A. Although these methods have been developed specifically for VINCI, they are easily applicable to other single-mode beam combiners, and to spectrally dispersed fringes.
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