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Institut für Astronomie und AstrophysikAbteilung AstronomieSand 1, D-72076 Tübingen, Germany |
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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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