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