... The purpose of the wide field (1.65o diameter in the IR) survey telescope and camera facility is to perform extensive surveys of the southern skies whose sensitivity is matched to the needs of today's 8-m class telescopes. ...
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Ссылки http://www.vista.ac.uk/Files/docs/VISTA_in_eso-messenger-no117.pdf -- 919.4 Кб -- 14.06.2012 Похожие документы
... 7. D.L. Terrett, et al., "Active optics and autoguiding control for VISTA", Proc SPIE 5496 p.129 (2004). 8. M. Caldwell et al., ... 8. M. Caldwell et al., "Aspects of concurrent design during the VISTA IR camera detailed design phase". ...
... 8 Mpixels 268.4 Mbytes 67.1 Mbytes 1 pawprint every 10 sec 26.8 Mbytes per second 14 ... M. McPherson, A. Born, W. Sutherland, J. Emerson, "The VISTA Project: a review of ...
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Ссылки http://www.vista.ac.uk/Files/docs/vdfs/spie-5493-30_VDFS-Overview.pdf -- 144.7 Кб -- 20.04.2011 Похожие документы
... 8 of 21 Calibration Pipeline Data Flow System · Removes instrumental artefacts · Combine pawprints component exposures offset by small jitters · Calibrates each pawprint photometrically and astrometrically · Provides Quality Control measures · See Jim ...
... pixels either side, where m is the interleave factor m x m from microstepping e.g ... A.M. Chavan, F. Comeron, M. Peron, T. Canavan, D. Dorigo, and P. Nunes "From ... M.J. Irwin et al 2006 in preparation A. Lawrence, S.J. Warren, O. Almaini, A.C. Edge ...
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Ссылки http://www.vista.ac.uk/Files/docs/vdfs/6270_30_VDFSStatus.PDF -- 611.9 Кб -- 14.06.2012 Похожие документы
... VISTA is a 4-m class wide field survey telescope for the southern hemisphere ... 8 hours per night in even periods (summer, 1 October to end of February). ... 6.70 . 5.275 . 35.343 . Diagonal (unfilled pawprint) 8.5273 dets . Tile . ...