Is a web service which calculates an astrometric solution for an image. So basically matches stars in the frame to star catalogues and added to WCS information to the fits file. This guide outlines taking a frame from an observation and get a new fits file that is calibrated (including plate scale).

-- Public.StewartBoogert - 08 Jan 2016
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Physics WebpagesRHUL WebpagesCampus Connect • Royal Holloway, University of London, Egham, Surrey TW20 0EX; Tel/Fax +44 (0)1784 434455/437520

Topic revision: r3 - 31 Jan 2016 - StewartBoogert

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