A New Intrared Top-end for the 3.6 m Telescope

Details A New Intrared Top-end for the 3.6 m Telescope A New Intrared Top-end for the 3.6 m Telescope

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978msngr..13...23.&link_type=abstract

The Messenger, vol. 13, p. 23-24

Computer Science

Scientific paper

So far, most, but not all, infrared observations have been carried out with conventional optical telescopes. This often implies that a comparatively strong infrared radiation (heat) from the telescope proper has to be subtracted from the total signal for a given celestial infrared source. This is particularly so when the telescope has much material in the beam, e. g. support of the secondary mirror, cables, etc.

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