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:|
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:firstname.lastname@example.org