#529 - imposing isotropy or at least N-fold symmetry on correlated noise

This pull request is for some small additional functionality in the handling of correlated noise, which is parallel to the whitening functionality that was already in place but involves imposing N-fold symmetry on the noise (without making it white).  Here N is some even integer >=4, with the default choice being 4, likely the lowest order of symmetry necessary to avoid weird shear systematics due to anisotropic correlated noise.

In general, the amount of noise that has to be added is substantially less than what has to be added to make correlated noise in COSMOS images fully white.  So that would be the main motivation for doing this instead of whitening.

Based on some discussion on #529, the ```applyWhiteningTo()``` method has been changed to ```whitenImage()```, parallel to the new ```symmetrizeImage()``` (though ```applyWhiteningTo()``` still works for now).   Mike put the new symmetrizing option into config, and moved the existing whitening option in config from being an attribute of the real galaxies to being specified at the same time as the noise in the final image.  (Mike, should we update the config wiki once this is merged?  Or did we decide the wiki was going to correspond to the latest tagged version?)

@emhuff , this should be helpful for you...
That's a possibility.  But it would probably be better to have different names.  

If we go with preferring the image-based methods, then I think it's ok to have the noise methods have unwieldy names.  We can even go back to the original `applyWhiteningTo` name and just prefer `image.whitenNoise(noise)`.  Then some other possibly unwieldy name for the noise method (like `noise.symmetrizeNoiseInImage(image)` or `noise.applySymmetrizationOfNoiseTo(image)`) would be equivalent to the preferred `image.symmetrizeNoise(noise)`.