DRAGyS -- A comprehensive tool to extract scattering phase functions in protoplanetary disks
Maxime Roumesy, Fran\c{c}ois M\'enard, Ryo Tazaki, Gaspard Duch\^ene, Laurine Martinien, R\'emi Zerna

TL;DR
DRAGyS is a new, efficient tool that extracts scattering phase functions from protoplanetary disk images without complex modeling, enabling large-scale dust property analysis.
Contribution
It introduces a fast, geometrical method to derive disk parameters and SPF directly from images, bypassing radiative transfer modeling limitations.
Findings
DRAGyS accurately recovers disk geometry and SPF from synthetic images.
It accounts for limb brightening effects, improving dust property inference.
The tool is validated on real disk images, showing consistent results.
Abstract
The early stages of planet formation, involving dust grain growth and planetesimals formation, remain shrouded in mystery. The analysis of the Scattering Phase Function (SPF) measured in disks surrounding young stars holds great potential for revealing crucial information about dust grain properties. Given the increasing number of high-quality datasets available, an efficient method to extract the SPF is required. DRAGyS is a tool designed for the quick and comprehensive analysis of ring-shaped protoplanetary disks. It directly estimates the disk geometry and extracts the total and polarized SPF from scattered light images, without requiring any radiative transfer modeling, a limitation of previous efforts. Key disk parameters (inclination, position angle, aspect ratio) are obtained by fitting ellipses to the disk intensity peaks from the ring surface, assuming the disks are circular.…
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Taxonomy
TopicsAstro and Planetary Science · Astrophysics and Star Formation Studies · Spacecraft and Cryogenic Technologies
