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dc.contributor.authorChapman, S. C.en_US
dc.contributor.authorBurley, G. S.en_US
dc.contributor.authorWalker, G. A. H.en_US
dc.date.accessioned2014-03-12T19:21:06Z
dc.date.available2014-03-12T19:21:06Z
dc.date.issued1997-06-26en_US
dc.identifier.citationChapman, S. C., G. S. Burley, and G. A. H. Walker. 1997. "First results from the UBC etch-alignment mosaic CCD." SPIE 3019en_US
dc.identifier.issn1996-756X
dc.identifier.urihttp://hdl.handle.net/10222/45507
dc.description.abstractFirst imaging results are obtained with a new CCD mosaic prototype (3K x 3k, 15 \mu m pixels). The CCDs are aligned using an etched socket alignment technique. Three different measurements of the alignment are made using star images, test p attern images, and microscope analysis. The CCDs have an angular misalignement o f less than 30 ppm. The composite device is flat to within \pm 3 \mu m, with rows/columns oriented to within 20 ppm. The use of an existing technology with built in precision reduces many of the difficulties and expenses typically encountered with mosaic detector construction. A new camera being built for the UBC liquid mirror telescope is al so described.en_US
dc.description.urihttp://dx.doi.org/10.1117/12.275186
dc.relation.ispartofSPIE
dc.titleFirst results from the UBC etch-alignment mosaic CCDen_US
dc.title.alternativearXiv:astro-ph/9706267en_US
dc.typearticleen_US
dc.identifier.volume3019
dc.identifier.startpageen_US
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