UNAM scanning Fabry-Perot interferometer (PUMA) for the study of interstellar medium

Details UNAM scanning Fabry-Perot interferometer (PUMA) for the study of interstellar medium UNAM scanning Fabry-Perot interferometer (PUMA) for the study of interstellar medium

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994spie.2198..409l&link_type=abstract

Proc. SPIE Vol. 2198, p. 409-412, Instrumentation in Astronomy VIII, David L. Crawford; Eric R. Craine; Eds.

Astronomy and Astrophysics

Astronomy

Scientific paper

The system called PUMA is an instrument consisting of a focal reducer coupled to a scanning Fabry-Perot interferometer (SFPI), which is being developed for the Observatorio Astronomicao Nacional at San Pedro Martir, B.C. It will be installed at the 2.0 m Ritchey-Chretien telescope with a focal ratio of F/7.9. It has interference filters, a calibration system, and field diaphragms. The SFPI can be moved out of the optical path in order to acquire direct images. The images produced by this instrument will be focused on an optoelectronic detector, a CCD, or a Mepsicron, depending on the spectral range used.

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