PyMorph: Automated galaxy structural parameter rstimation using python

dc.contributor.authorVikram, Vinu
dc.contributor.authoret al.
dc.contributor.authorWadadekar, Yogesh
dc.contributor.authorKembhavi, A.K.
dc.date.accessioned2012-03-04T12:49:24Z
dc.date.available2012-03-04T12:49:24Z
dc.date.issued2010-07-20
dc.description.abstractWe 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.en_US
dc.identifier.urihttp://hdl.handle.net/11007/307
dc.language.isoenen_US
dc.relation.ispartofseriesIUCAA Preprints;18/2010
dc.subjectGalaxiesen_US
dc.subjectPhotometry — Galaxiesen_US
dc.subjectEormation — Galaxiesen_US
dc.subjectEvolution — Galaxiesen_US
dc.subjectFundamental Parametersen_US
dc.titlePyMorph: Automated galaxy structural parameter rstimation using pythonen_US
dc.typeArticleen_US

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