Vikram, Vinuet al.Wadadekar, YogeshKembhavi, A.K.2012-03-042012-03-042010-07-20http://hdl.handle.net/11007/307We present a new software pipeline – PyMorph – for automated estimation of structural parameters of galaxies. Both parametric fits through a two dimensional bulge disk decomposition as well as structural parameter measurements like concentration, asymmetry etc. are supported. The pipeline is designed to be easy to use yet flexible; individual software modules can be replaced with ease. A find-and-fit mode is available so that all galaxies in a image can be measured with a simple command. A parallel version of the Pymorph pipeline runs on computer clusters and a Virtual Observatory compatible web enabled interface is under development.enGalaxiesPhotometry — GalaxiesEormation — GalaxiesEvolution — GalaxiesFundamental ParametersArticle