An interferometer consisting entirely of optically contacted optical elements is described. The interferometer is part of a system to measure the p-mode oscillations of stars from the Doppler signal on a fringe, in the visible.
© 2003 Optical Society of America
J. Maillard, B. Mosser, and J. Reess, " SIAMOIS: A monolithic visible interferometer for stellar seismology," in Fourier Transform Spectroscopy, A. Sawchuk, ed., Vol. 84 of OSA Trends in Optics and Photonics (Optical Society of America, 2003), paper FThA3.
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