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ELLFOU and ELLPRO work in very different ways. ELLPRO works by creating
trial ellipses which it places on the galaxy. It then carefully adjusts the
shape and position of the ellipses until the brightness variation around
the ellipse is minimised. ELLFOU identifies the locations of all the
pixels in a given isophotal range, takes a subset of those and then trys to
fit an ellipse through the pixels that minimises the pixel/ellipse distance
sum. These approaches are known as intensity and contour analysis respectively.
You might well ask then why two routines are provided. The reason is simply that
galaxies vary enormously. If these routines are used with a normal galaxy
of approximately elliptical shape they will normally both behave well. But
this is not always the case. Limits to this sensible behaviour are
outlined below.
Next: Limitations of ELLPRO and ELLFOU
Up: ESP Extended Surface Photometry
Previous: Profiling galaxies using contour analysis
ESP --- Extended Surface Photometry
Starlink User Note 180
Norman Gray
Mark Taylor
Grant Privett
27 January 2000
E-mail:ussc@star.rl.ac.uk
Copyright © 2002 Council for the Central Laboratory of the Research Councils