ABSTRACT The Spitzer Survey of Stellar Structure in Galaxies (S 4 G) is the largest
available database of deep, homogeneous middle-infrared (mid-IR) images of galaxies of all …

We revisit the bimodal distribution of the galaxy population commonly seen in the local
universe. Here, we address the bimodality observed in galaxy properties in terms of spectral …

Testing theories of hierarchical structure formation requires estimating the distribution of
galaxy morphologies and its change with redshift. One aspect of this investigation involves …

Visual inspections of the first optical rest-frame images from JWST have indicated a
surprisingly high fraction of disk galaxies at high redshifts. Here, we alternatively apply self …

Interactions between galaxies leave distinguishable imprints in the form of tidal features,
which hold important clues about their mass assembly. Unfortunately, these structures are …

We have derived disc scalelengths for 30 374 non-interacting disc galaxies in all five Sloan
Digital Sky Survey (SDSS) bands. Virtual Observatory methods and tools were used to …

In this paper we present a new statistic for quantifying galaxy morphology based on
measurements of the Gini coefficient of galaxy light distributions. This statistic is easy to …

We present a method for automatic detection and classification of galaxies which includes a
novel data-augmentation procedure to make trained models more robust against the data …

We explore unsupervised machine learning for galaxy morphology analyses using a
combination of feature extraction with a vector-quantized variational autoencoder (VQ-VAE) …

The amount and complexity of data delivered by modern galaxy surveys has been steadily
increasing over the past years. New facilities will soon provide imaging and spectra of …