Final tests and commissioning of the UCL echelle spectrograph

1990; SPIE; Volume: 1235; Linguagem: Inglês

10.1117/12.19119

ISSN

1996-756X

Autores

Francisco Diego, Andrew Charalambous, A. C. Fish, David Walker,

Tópico(s)

Adaptive optics and wavefront sensing

Resumo

The optical design and performance of the UCLES echelle spectrograph, installed at the f/37.7 coude focus of the 3.9-m AAT in June 1988, are described and illustrated with extensive diagrams, drawings, photographs, and sample spectra. The UCLES operates at 300-1100 nm with resolution 30,000-115,000 and adjustable collimated beam size; it employs either 31.6-g/mm or 79-g/mm echelle gratings and a train of UV-transmitting fused-silica prisms for cross-dispersion. Also discussed are the focal modifier lenses; the Bowen-Walraven image slicer; the commissioning procedures; and preliminary observations of Zeta Oph, planetary nebulae, and Seyfert galaxies.

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