Integration of visible CCDs into cryogenically cooled dewars for astronomical applications

Details Integration of visible CCDs into cryogenically cooled dewars for astronomical applications Integration of visible CCDs into cryogenically cooled dewars for astronomical applications

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986spie..627..176a&link_type=abstract

IN: Instrumentation in astronomy VI; Proceedings of the Meeting, Tucson, AZ, Mar. 4-8, 1986. Part 1 (A87-36376 15-35). Bellingha

Astronomy and Astrophysics

Astronomy

1

Charge Coupled Devices, Cryogenic Equipment, Equipment Specifications, Telescopes, Functional Design Specifications, Retrofitting, Temperature Control, Thermal Stability, Upgrading

Scientific paper

The introduction of large area arrays provides new technical challenges in the retro-fit of existing astronomical instrument dewars and in the design of new dewars. The evolutionary implementation of cryogenically cooled dewars for visible CCDs at NOAO is described. The performance specifications required by applications in ground-based astronomy are discussed. Various dewar designs are presented and performance characteristics are given where applicable.

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