Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE · 2000 · 11 citations · 0 references
Natural SciencesAstronomyPhysicsAstrophysicsOpticsSpectroscopyInfrared InstrumentationInfrared TelescopesInterferometryNear-infrared AstronomyOptical InstrumentationSpace-based Infrared ObservatoriesCombiner DesignInterferometric InstrumentationMichelson InterferometerOptical DesignOptical InterferometersOptical Path Difference MeasurementOptical Path LengthStellar Interferometry
We have built an infrared beam combiner for the GI2T/REGAIN interferometer of the Observatoire de la Cote d'Azur. The beam controller allows us to record spectrally dispersed Michelson interference fringes in the near-infrared J-, H- or K-bands. The beam combiner has the advantage that Michelson interferograms can simultaneously be recorded in about 128 different spectral channels. The tilt of the spectrally dispersed fringes is a measure of the instantaneous optical path difference. We present the optical design of the beam combiner and GI2T/REGAIN observations of the Mira star R Cas with this beam combiner in the spectral range of 2.00 micrometers - 2.18 micrometers (observations on 22 and 25 August 1999; variability phase 0.08; V-magnitude approximately 6; seven baselines between 12 m and 24 m; reference stars Vega and (beta) Peg).