ELLIPSECT: A surface brightness analysis tool for GALFIT 3

Fuente: arXiv
Guardado en:
Detalles Bibliográficos
Autores principales: Añorve, Christopher, Reyes-Amador, Omar Ulises, Ríos-López, Emmanuel, Tadeo, Diego de Ramón, López-Cruz, Omar
Formato: Preprint
Publicado: 2025
Materias:
Acceso en línea:
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
_version_ 1866914362232406016
author Añorve, Christopher
Reyes-Amador, Omar Ulises
Ríos-López, Emmanuel
Tadeo, Diego de Ramón
López-Cruz, Omar
author_facet Añorve, Christopher
Reyes-Amador, Omar Ulises
Ríos-López, Emmanuel
Tadeo, Diego de Ramón
López-Cruz, Omar
contents EllipSect is a user-friendly analysis and measurement tool, implemented in Python, that operates on the imaging data together with the output of the widely used 2D surface-brightness fitting code GALFIT 3. It produces publication-quality figures and exportable data products to enable quantitative assessment of GALFIT 3 models and their individual components. In addition, EllipSect computes non-parametric measurements that are not provided by GALFIT 3, including the total effective radius resulting from multi-component fits, cusp radius, and the Petrosian radius. This paper provides examples and a quick guide for EllipSect.
format Preprint
id arxiv_https___arxiv_org_abs_2501_10079
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle ELLIPSECT: A surface brightness analysis tool for GALFIT 3
Añorve, Christopher
Reyes-Amador, Omar Ulises
Ríos-López, Emmanuel
Tadeo, Diego de Ramón
López-Cruz, Omar
Instrumentation and Methods for Astrophysics
EllipSect is a user-friendly analysis and measurement tool, implemented in Python, that operates on the imaging data together with the output of the widely used 2D surface-brightness fitting code GALFIT 3. It produces publication-quality figures and exportable data products to enable quantitative assessment of GALFIT 3 models and their individual components. In addition, EllipSect computes non-parametric measurements that are not provided by GALFIT 3, including the total effective radius resulting from multi-component fits, cusp radius, and the Petrosian radius. This paper provides examples and a quick guide for EllipSect.
title ELLIPSECT: A surface brightness analysis tool for GALFIT 3
topic Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2501.10079