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This work studies the compactness of galaxies in the early Universe during the epoch of reionization. Using cosmological simulations, we explore galaxy compaction as a possible formation channel for extremely compact systems such as the recently observed little red dots.
Recommended citation: Cataldi et. al. (2024) https://ganegroup.github.io/workshop/Workshop_on_Massive_stars
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This work studies the populations of X-ray binaries in local galaxies.
Recommended citation: Pellizza et. al. (2024) https://ui.adsabs.harvard.edu/abs/2025BAAA...66..377P/abstract
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We develop methods to classify X-ray binaries using only X-ray observational data. The study explores how different X-ray properties can be used to distinguish binary populations in nearby galaxies.
Recommended citation: Badaracco et. al. (2024) https://ui.adsabs.harvard.edu/abs/2025BAAA...66..401B/abstract
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This article analyze the dark matter (dm) halo evolution through time. For this study we use a Milky Way like haloes subsample from CIELO (ChemodynamIcal propertiEs of gaLaxies and the cOsmic web) project. This project aims at studying the formation of galaxies in different environments using zoom-ins simulations.
Recommended citation: Cataldi et al. (2023b) https://ui.adsabs.harvard.edu/abs/2023BAAA...64..178C/abstract