NAME: astrd2xy PURPOSE: Astrometry conversion from ($\alpha$,$\delta$) to image (x,y) DESCRIPTION: This transformation can either be based on a simple linear transformation with rotation from the celestial sphere to linear CCD chip coordinates. Or, it can use a full astrometric solution (including linear). CATEGORY: Astrometry CALLING SEQUENCE: astrd2xy,ra,dec,info,x,y INPUTS: ra - Right ascension (radians) dec - Declination (radians) info - Transformation information held in an anonymous structure. There are two different groups of tags that can appear. The original simple linear transformation needs the following tags: pscale - Plate scale (arcsec/pixel). rang - Rotation angle of image (radians). xflip - -1 if image flipped in X, 1 if not. yflip - -1 if image flipped in Y, 1 if not. The full-up transformation requires a different set of tags: renormfac - normalization factor cxi - xi transformations coefficients (x,y -> xi) ceta - eta transformations coefficients (x,y -> eta) terms - string array with names of terms to fit Both types need the following. xcref - X center of image. ycref - Y center of image. raref - Right ascension of center of image (tangent plane). decref - Declination of center of image (tangent plane). OPTIONAL INPUT PARAMETERS: KEYWORD INPUT PARAMETERS: FULL - Flag, if set indicates the full transformation should be used. Only the tags needed must be provided. OUTPUTS: x - X coordinate in image y - Y coordinate in image KEYWORD OUTPUT PARAMETERS: COMMON BLOCKS: SIDE EFFECTS: RESTRICTIONS: PROCEDURE: MODIFICATION HISTORY: 1997/04/05 - Written by Marc W. Buie, Lowell Observatory 2009/06/21, MWB added full-up transformation 2009/11/02, MWB, split off most of code into astsn2xy