Computational
Galaxy Formation &
Large-Scale Structures

Over recent years, the Spanish community working on computational studies of galaxy formation and large-scale structure has reached a level of maturity and critical mass that motivates the creation of a dedicated forum within the SEA meeting. This symposium aims to bring together researchers involved in state-of-the-art numerical simulations across a wide range of scales, from high-resolution models of galaxy internal physics to next-generation cosmological volumes reproducing the cosmic web.

The symposium will provide a platform to:

• Present recent scientific results in galaxy formation and numerical cosmology

• Foster scientific and technical synergies between groups

• Encourage new national and international collaborations

• Highlight methodological advances, including machine learning, advanced data analysis, and alternative cosmological models

Topics will include (but are not limited to): dwarf galaxies, spiral galaxies, the Local Group, galaxy clusters, large-scale structure, comparisons with major observational surveys (e.g. Euclid, DESI, Gaia), and simulations in non-standard cosmological frameworks.

The symposium is planned to consist of three 1.5/2 hours blocks, including two introductory reviews, invited focused talks and contributed presentations. 

Both oral contributions and e-posters will be accepted.

Scientific Organising Committee (SOC)

•     Arianna Di Cintio (Universidad de La Laguna / IAC) — Chair

•     José Oñorbe Bernis (Universidad de Sevilla) — Co-Chair

•     Susana Planelles (Universitat de València)

•     Raúl Angulo (DIPC, Donostia / Ikerbasque)

•     Daniel Ceverino Rodríguez (Universidad Autónoma de Madrid)

See you in Tarragona!