Results 111 to 120 of about 11,134,879 (212)
How Dust Models Shape High-z Galaxy Morphology: Insights from the NewCluster Simulation
Dust plays a pivotal role in shaping the observed morphology of galaxies. While traditional cosmological simulations often assume a fixed dust-to-gas or dust-to-metal (DTM) mass ratio to model dust effects, recent advancements have enabled on-the-fly ...
Gyeong-Hwan Byun +12 more
doaj +1 more source
The Hot and Energetic Universe:The evolution of galaxy groups and clusters [PDF]
Major astrophysical questions related to the formation and evolution of structures, and more specifically of galaxy groups and clusters, will still be open in the coming decade and beyond: what is the interplay of galaxy, supermassive black hole, and ...
Bourdin, H. +47 more
core
Galaxies Going Bananas: Inferring the 3D Geometry of High-redshift Galaxies with JWST-CEERS
The 3D geometries of high-redshift galaxies remain poorly understood. We build a differentiable Bayesian model and use Hamiltonian Monte Carlo to efficiently and robustly infer the 3D shapes of star-forming galaxies in James Webb Space Telescope Cosmic ...
Viraj Pandya +55 more
doaj +1 more source
Star–galaxy classification in deep LSST data with random forest
Context. The Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) will produce unprecedentedly deep and wide photometric catalogues, enabling transformative studies of faint stellar systems such as the research of ultra-faint dwarf (UFD ...
Gatto M. +4 more
doaj +1 more source
Automating Galaxy Image Classification in Galaxy Zoo:A Comparative Study of Deep Learning Models
This study compares the effectiveness of Artificial Neural Networks (ANNs) and Logistic Regression in classifying galaxy images from Galaxy Zoo 1. We propose Convolutional Neural Network (CNN) and Autoencoder models as potential solutions to mitigate the
Chiew, Soon Piin +2 more
core +1 more source
The physical processes responsible for shaping how galaxies form and quench over time leave imprints on both the spatial (galaxy morphology) and temporal (star formation history; SFH) tracers that we use to study galaxies.
Juan Pablo Alfonzo +10 more
doaj +1 more source
The morphologies of distant galaxies. 1: an automated classification system
Roberto G. Abraham +3 more
openaire +1 more source
Mass-to-light ratio of galaxy systems
We study the mass-to-light ratio of galaxy systems from poor groups to rich clusters. We extend a previous work based on 89 clusters obtaining blue luminosity and virial mass for other 52 clusters, 43 poor systems, and similar to 500 groups of two ...
G. Giuricin +4 more
core
Secondary evolution of galaxies investigated by N-body simulations [PDF]
In the ΛCDM cosmology, merging is one of the most important physical processes that drives the formation and evolution of galaxies. In the present work, we use N-body techniques to investigate some of currently open issues related to the formation and ...
Coppola, Giuseppina
core +1 more source
Identification and Analysis of Galactic Bars in DESI Legacy Imaging Surveys
We present a comprehensive study of bar structures in the local universe using data from the DESI Legacy Imaging Surveys. Through isophotal analysis of 232,142 galaxies, we identify bars and classify them into strong and weak categories based on ...
Wenwen Wang, Zhimin Zhou
doaj +1 more source

