Computer Science – Performance
Scientific paper
Jul 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010spie.7733e..29g&link_type=abstract
Ground-based and Airborne Telescopes III. Edited by Stepp, Larry M.; Gilmozzi, Roberto; Hall, Helen J. Proceedings of the SPIE,
Computer Science
Performance
Scientific paper
The QUIJOTE CMB experiment aims to characterize the polarization of the CMB in the frequency range 10-30 GHz and large angular scales. It will be installed in the Teide Observatory, following the projects that the Anisotropy of the Cosmic Microwave Background group has developed in the past (Tenerife experiment, IAC-Bartol experiment...) and is running at the present time (VSA, Cosmosomas). The QUIJOTE CMB experiment will consist of two telescopes which will be installed inside a unique enclosure, which is already constructed. The layout of both telescopes is based on an altazimuth mount supporting a primary and a secondary mirror disposed in a offset Gregorian Dragon scheme. The use of industrial-like fabrication techniques, such as sand-mould casting, CNC machining, and laser tracker measuring for alignment, provided the required performances for microwave observation. A fast-track construction scheme, altogether with the use of these fabrication techniques allowed designing and manufacturing the opto-mechanics of the telescope in 14 months prior to delivery for final start-up in December 2008.
Etxeita Borja
Genova Ricardo T.
Gomez Alberto
Gomez Francisca
Herreros José-Miguel
No associations
LandOfFree
QUIJOTE telescope design and fabrication does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with QUIJOTE telescope design and fabrication, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and QUIJOTE telescope design and fabrication will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1375965