A new configuration for spectroscopic survey telescope.

Details A new configuration for spectroscopic survey telescope. A new configuration for spectroscopic survey telescope.

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esoc...42..105w&link_type=abstract

ESO Conference on Progress in Telescope and Instrumentation Technologies, p. 105 - 108

Physics

Scientific paper

In this configuration, the primary mirror is 12.4 m long in east-west direction and 4 m wide. It can rotate round the east-west level axis. The primary mirror is spherical and consists of 94 mirrors with a diameter of each mirror of 0.75 m. For each object the useful area is 4 m on the primary mirror and the tracking time is one hour. The sum of simultaneously observable objects is about 2400. The effect of this telescope equals four telescopes, each having 4 m aperture.

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