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The CIELO Project

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The Chemo-dynamIcal propertiEs of gaLaxies and the cOsmic web, Project, CIELO, aims to study the chemical enrichment of baryons in galaxies across the cosmic web by using zoom-in galaxies in different environments. as part of the LACEGAL Network. CIELO was envisaged within LACEGAL and SAN Networks.

Members

and collaborators

Lucas Bignone (IAFE, Argentina)

R. Dominguez-Tenreiro (Universidad Autónoma de Madrid).

N. Padilla (IATE, Argentina)

S. Pedrosa (IAFE, Argentina)

P. Tissera (PUC, Chile)

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P. Cataldi (IAFE)

E. Sillero (PUC)

D. Barrientos (PUC)

C. Casanueva (PUC)

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Students:

J. Gonzalez (PUC)

V. Miranda (PUC)

I. Muñoz (PUC)

B. Tapia (PUC)

B. Silva (PUC)

L. Purcell (PUC)
 

Collaborators:

Rodriguez, S. S. Varela (PUC) & Lambas, D.G (IATE)

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The simulations

The CIELO have been designed to study the connection between galaxies and their environment across their history of formation. They are planned to include 20 high-resolution zoom-in galaxies selected from different environments. At the moment we have six of them which are being analysed for different projects.

GraduateThesis  using CIELO

Publications using CIELO

Catalina Casanueva: PhD 2025

Jenny Gonzalez: PhD 2025

Anell Cornejo: Msc 2024

Rodriguez et al. 2022: We study the impact of the environment on galaxies as they fall in and orbit in the potential well of a Local Group (LG) analogue, following them with high cadence (movies).

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Cataldi et al. 2023: In this work, we aim at investigating the morphology evolution of Milky Way mass-like dark matter haloes selected from the CIELO and ILLUSTRIS-TNG projects

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Gonzalez-Jara et al. 2024: We studied the assembly of stellar haloes and the characteristics of the accreted satellites and their chemical abundances.  

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Casanueva et al. 2024: We develop a model for Primordial Black Holes as a potential component of dark matter and explore their feedback effects on the properties of the gas before star formation occurs. 

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Tissera et al. 2025:We present the CIELO project and show the main observed relation determined by the CIELO galaxies.

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Cornejo et al. 2025:Mocking integral field unit observations and metallicity diagnostics from cosmological simulations.

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Tapia-Contreras et al. 2025: Insight into the physical processes that shape the metallicity profiles in galaxies.

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Muñoz-Escolbar et al. 2025: The mass-metallicity relation of bulges.

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