Institut für Astronomie und AstrophysikAbteilung AstronomieSand 1, D-72076 Tübingen, Germany |
TRIPP_DEFINE_MASK_AUTOHELP
Defines the mask of the image automatically for the number of sources defined in the logfile. Will define six background regions for each selected source.
Astronomical Photometry.
TRIPP_DEFINE_MASK_AUTOHELP, log,image,silent,$ BACK_POSX,BACK_POSY,BACK_SUM,BX,BY,CUT,$ HSIDE,ISIZE,IXH,IXL,IYH,IYL,$ JLOW,JHIGH,JOFFSET,$ RAD,SX,SY
logname : the reduction logfile name log : the reduction logfile variables image : the image for which a mask will be defined BACK_POSX : empty array needed for internal positioning of background fields BACK_POSY : empty array needed for internal positioning of background field BACK_SUM : empty array needed for internal positioning of background field CUT : defines rejection of background fields HSIDE : half length of mask background box ISIZE : image size IXH : highest pixel number in x direction IXL : lowest pixel number in xdirectio IYH : highest pixel number in y direction IYL : lowest pixel number in y direction RAD : extraction radii XPOS : x position of pivot point; make first entry in sx YPOS : y position of pivot point; make first entry in sy
silent : prevent screen output and disable
BX : x-coordinates of background fields with (6 * # sources) entries BY : y-coordinates of background fields with (6 * # sources) entries SX : x-coordinates of stars SY : y-coordinates of stars SNAME : Reference name/number of stars JLOW : index of faintest background field to use JHIGH : index of brightest background field to use JOFFSET : offset used to reorder array of background field positions equals 0 if 2 brightest bg fields are rejected equals 1 if brightest & faintest bg field rejected equals 2 if 2 faintest bg fields rejected
Version 1.0, 2004 , S.D. Huegelmeyer, S. Schuh 2006/03 S.S., obsoleted ccd_quad
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