TL;DR
AutoProf is an automated, non-parametric pipeline for extracting galaxy surface brightness profiles, offering improved accuracy and flexibility over existing methods, and capable of analyzing faint isophotes in large galaxy surveys.
Contribution
AutoProf introduces a novel automated non-parametric light profile extraction pipeline with fit-stabilization and advanced analysis features for galaxy images.
Findings
AutoProf reliably extracts fainter isophotes than other methods.
Two-component parametric fits are insufficient for high-fidelity galaxy modeling.
AutoProf outperforms existing photometry algorithms in accuracy and automation.
Abstract
We present an automated non-parametric light profile extraction pipeline called AutoProf. All steps for extracting surface brightness (SB) profiles are included in AutoProf, allowing streamlined analyses of galaxy images. AutoProf improves upon previous non-parametric ellipse fitting implementations with fit-stabilization procedures adapted from machine learning techniques. Additional advanced analysis methods are included in the flexible pipeline for the extraction of alternative brightness profiles (along radial or axial slices), smooth axisymmetric models, and the implementation of decision trees for arbitrarily complex pipelines. Detailed comparisons with widely used photometry algorithms (photutils, XVISTA, and GALFIT) are presented. These comparisons rely on a large collection of late-type galaxy images from the PROBES survey. The direct comparison of SB profiles shows that…
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