Gradient Pattern Analysis Applied to Galaxy Morphology

Gradient pattern analysis (GPA) is a well-established technique for measuring gradient bilateral asymmetries of a square numerical lattice. This paper introduces an improved version of GPA designed for galaxy morphometry. We show the performance of the new method on a selected sample of 54,896 objects from the SDSS-DR7 in common with Galaxy Zoo 1 catalog. The results suggest that the second gradient moment, G2, has the potential to dramatically improve over more conventional morphometric parameters. It separates early from late type galaxies better (\sim 90%) than the CAS system (C \sim 79%, A \sim 50%, S \sim 43%) and a benchmark test shows that it is applicable to hundreds of thousands of galaxies using typical processing systems.