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Data reduction methods for single-mode optical interferometry - Application to the VLTI two-telescopes beam combiner VINCI
P. Kervella, D. Segransan, V. Coude du Foresto
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…
Cepheid distances from infrared long-baseline interferometry - II. Calibration of the Period-Radius and Period-Luminosity relations
P. Kervella, D. Bersier, D. Mourard +2
Using our interferometric observations of seven classical Cepheids reported in Kervella et al. (2003, Paper I), complemented by previously existing measurements, we derive new cali…
The angular size of the Cepheid L Car: a comparison of the interferometric and surface brightness techniques
P. Kervella, P. Fouque, J. Storm +5
Recent interferometric observations of the brightest and angularly largest classical Cepheid, L Carinae, with ESO's VLT Interferometer (VLTI) have resolved with high precision the…
Interferometric observations of the supergiant stars alpha Orionis and alpha Herculis with FLUOR at IOTA
G. Perrin, S. T. Ridgway, V. Coudé du Foresto +3
We report the observations in the K band of the red supergiant star alpha Orionis and of the bright giant star alpha Herculis with the FLUOR beamcombiner at the IOTA interferometer…