Institut für Astronomie und AstrophysikAbteilung AstronomieSand 1, D-72076 Tübingen, Germany |
TRIPP_FLUX
Integrates flux in circular or rectangular aperture centered on xcen, ycen. See following descriptions for details of centering and subpixels.
Astronomical Photometry.
TRIPP_FLUX, ima, rad ,xcen ,ycen , MAXINT=maxint, $ [ flux, area, SUB=sub, QUAD=quad, SILENT=silent, $ N_SIGMA=n_sigma ]
IMA : 2D image array. RAD : Radius of circular aperture [pixel] for flux integration. X/YCEN : Center of aperture, (0,0) is lower left corner of lower left pixel in frame.
NONE.
NONE.
SUB : Number of subpixels = sub^2 for division of original pixel, defaulted to 5. QUAD : Use rectangle with area [2*rad+1]^2 instead of circle. NOTE - in QUAD mode, the quadrangle includes only whole pixels (speed), therefore the center of the mask may be shiftet by a fraction of a pixel in x/y and rad is converted to an integer. N_SIGMA : Cut value for sigma filtering (IF /QUAD SET ONLY) aperture, see CCD_BFILT.
FLUX : Integrated flux in the defined aperture. AREA : Area in defined aperture [original (not subdivided) pixels].
MAXINT : Max. Intensity [ADU] in aperture.
NONE.
Uses CCD_ZOOM, deletes and opens new window device 0, if /SILENT is not set.
SATURATED PIXEL ARE DEFINED AS THOSE ABOVE 65000. !
Ralf D. Geckeler - %CCD% package for IDL - written Sept.96. original name was ccd_flux Stefan Dreizler - 12/1999: use median of background instead of mean
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