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: http://jet.sao.ru/hq/lsfvo/devices/scorpio/ifp/ifpmain.html
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The desired spectral range is cut out with the aid of interference filters with a FWHM=10-15 A, placed in the filter wheel near the focal plane. | |
For SCORPIO-IFP data reduction see:
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The device has been developed jointly by SAO and the
Interferometry Laboratory (Dr.J.Boulesteix) of the Marseille
Observatory (France). We use the piezo-tuned scanning Fabry-Perot Interferometer, produce by
Queensgate Instruments. Equipment status: guiest equipment. All observation performed with IFP are under supervision and in collaboration with staff of Laboratory of Spectroscopy and photometry of extragalactic objects. Laboratory Head: Dr. S.N. Dodonov, e-mail:dodo@sao.ru IFP responsible astronomer: A.V. Moiseev e-mail:moisav@sao.ru |