I am currently working with astronomical data among which I have comet images. I would like to remove the background sky gradient in these images due to the time of capture (twilight). The first program I developed to do so took user selected points from Matplotlib's "ginput" (x,y) pulled the data for each coordinate (z) and then gridded the data in a new array with SciPy's "griddata."
Since the background is assumed to vary only slightly, I would like to fit a 3d low order polynomial to this set of (x,y,z) points. However, the "griddata" does not allow for an input order:
griddata(points,values, (dimension_x,dimension_y), method='nearest/linear/cubic')
Any ideas on another function that may be used or a method for developing a leas-squares fit that will allow me to control the order?
Griddata uses a spline fitting. A 3rd order spline is not the same thing as a 3rd order polynomial (instead, it's a different 3rd order polynomial at every point).
If you just want to fit a 2D, 3rd order polynomial to your data, then do something like the following to estimate the 16 coefficients using all of your data points.