activity
20172026
most citedMachine and Deep Learning Applied to Galaxy Morphology -- A Comparative Study

93 citations · 175 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2026

SAGUI: SED-based Segmentation of Multi-band Galaxy Images -- Application to JADES in GOODS-South

Rafael S. de Souza, Andressa Wille, Shravya Shenoy +11

We present sagui, a modular framework for the analysis of multi-band imaging data in spatially resolved galaxies, with synergies to integral-field spectroscopy (IFS). Building on t…

astro-ph.IM2024★ 11 cited

Unveiling Galaxy Morphology through an Unsupervised-Supervised Hybrid Approach

I. Kolesnikov, V. M. Sampaio, R. R. de Carvalho +4

Galaxy morphology offers significant insights into the evolutionary pathways and underlying physics of galaxies. As astronomical data grows with surveys such as Euclid and Vera C.…

astro-ph.IM2019★ 93 cited

Machine and Deep Learning Applied to Galaxy Morphology -- A Comparative Study

P. H. Barchi, R. R. de Carvalho, R. R. Rosa +7

Morphological classification is a key piece of information to define samples of galaxies aiming to study the large-scale structure of the universe. In essence, the challenge is to…

astro-ph.GA2018★ 25 cited

Gradient Pattern Analysis Applied to Galaxy Morphology

Reinaldo. R. Rosa, Reinaldo. R. de Carvalho, Rubens. A. Sautter +6

Gradient pattern analysis (GPA) is a well-established technique for measuring gradient bilateral asymmetries of a square numerical lattice. This paper introduces an improved versio…

astro-ph.GA2017★ 35 cited

Investigating the Relation between Galaxy Properties and the Gaussianity of the Velocity Distribution of Groups and Clusters

R. R. de Carvalho, A. L. B. Ribeiro, D. Stalder +3

We investigate the dependence of stellar population properties of galaxies on group dynamical stage for a subsample of Yang catalog. We classify groups according to their galaxy ve…

astro-ph.GA2017★ 11 cited

Improving galaxy morphology with machine learning

P. H. Barchi, F. G. da Costa, R. Sautter +4

This paper presents machine learning experiments performed over results of galaxy classification into elliptical (E) and spiral (S) with morphological parameters: concetration (CN)…