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arXiv · 1007.4965

PyMorph: Automated Galaxy Structural Parameter Estimation using Python

Vinu Vikram·Yogesh Wadadekar·Ajit K. Kembhavi·G. V. Vijayagovindan
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Abstract

We 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.

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Vinu Vikram, Yogesh Wadadekar, Ajit K. Kembhavi, G. V. Vijayagovindan. 2010-07-28. PyMorph: Automated Galaxy Structural Parameter Estimation using Python. https://doi.org/10.1111/j.1365-2966.2010.17426.x

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