A simple prescription for simulating and characterizing gravitational arcs
Cristina Furlanetto, Bas\'ilio X. Santiago, Mart\'in Makler, Cl\'ecio, de Bom, Carlos H. Brandt, Angelo Fausti Neto, Pedro C. Ferreira, Luiz, Nicolaci da Costa, Marcio A. G. Maia

TL;DR
This paper introduces simple models and tools for simulating, detecting, and analyzing gravitational arcs in astronomical images, aiding large-scale surveys and arc characterization.
Contribution
It presents the ArcEllipse model, PaintArcs code, and ArcFitting tool, enabling automated simulation and fitting of gravitational arcs with validation on real data.
Findings
ArcEllipse model recovers total signal within 10-30%
Models automatically estimate length-to-width ratios
Residuals reveal arc substructures and merging effects
Abstract
Simple models of gravitational arcs are crucial to simulate large samples of these objects with full control of the input parameters. These models also provide crude and automated estimates of the shape and structure of the arcs, which are necessary when trying to detect and characterize these objects on massive wide area imaging surveys. We here present and explore the ArcEllipse, a simple prescription to create objects with shape similar to gravitational arcs. We also present PaintArcs, which is a code that couples this geometrical form with a brightness distribution and adds the resulting object to images. Finally, we introduce ArcFitting, which is a tool that fits ArcEllipses to images of real gravitational arcs. We validate this fitting technique using simulated arcs and apply it to CFHTLS and HST images of tangential arcs around clusters of galaxies. Our simple ArcEllipse model…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Gamma-ray bursts and supernovae · Radio Astronomy Observations and Technology
