Actualidad
Eventos
Agenda
Academic Spanish Course for Foreigners (2025)
Academic Spanish Course for Foreigners (2025)
The assembly process of star clusters: ALMA-IMF protoclusters traced by N2H+
The assembly process of star clusters: ALMA-IMF protoclusters traced by N2H+
Asymmetrical Post-main-sequence Nebulae 9
Asymmetrical Post-main-sequence Nebulae 9
Magnetic fields on Extrasolar Planets: From Radio Emission to High-Energy Cosmic Rays
Magnetic fields on Extrasolar Planets: From Radio Emission to High-Energy Cosmic Rays
Eighth Workshop on Robotic Autonomous Observatories
Eighth Workshop on Robotic Autonomous Observatories
SO Basics of Neural Networks 2025
SO Basics of Neural Networks 2025
WST: The Wide Field Spectroscopic Telescope
WST: The Wide Field Spectroscopic Telescope
Archivo
A UV-to-IR view of a nearby high-z analog with JWST and HST to interpret the first galaxies
A UV-to-IR view of a nearby high-z analog with JWST and HST to interpret the first galaxies
Dr. Matilde Mingozzi
Space Telescope Science Institute, Baltimore, USA
New clues about how Mars lost its water
New clues about how Mars lost its water
Dr. Gabriella Gilli
IAA-CSIC
¿Estamos solos en el universo? En busca de mundos habitables más allá del Sistema Solar
¿Estamos solos en el universo? En busca de mundos habitables más allá del Sistema Solar
Francisco Pozuelos
Instituto de Astrofísica de Andalucía (IAA-CSIC)
SO Colloquium: The multiple aspects of Star-Planet Interactions
SO Colloquium: The multiple aspects of Star-Planet Interactions
Dr. Rim Fares
United Arab Emirates University, UAE
Contar la contaminación lumínica de costa a costa
Contar la contaminación lumínica de costa a costa
SO Colloquium: What can we expect and hope for in quantum computing?
SO Colloquium: What can we expect and hope for in quantum computing?
Dr. Michael Hartmann
Institute of Theoretical Physics, Friedrich-Alexander Universität Erlangen-Nürnberg
Towards an observationally motivated AGN dusty torus model
Towards an observationally motivated AGN dusty torus model
Ulises Reyes Amador
IRYA-UNAM, México
El SKAO, un balcón al Universo con el corazón en la Tierra
El SKAO, un balcón al Universo con el corazón en la Tierra
Lourdes Verdes-Montenegro
Instituto de Astrofísica de Andalucía (IAA-CSIC)
SO Colloquium: The PARSEC view of star formation and the interstellar medium in galaxies
SO Colloquium: The PARSEC view of star formation and the interstellar medium in galaxies
Dr. Almudena Prieto
Instituto Astrofisica Canarias & University Observatory of Munich
Jets in Planetary Nebulae
Jets in Planetary Nebulae
Dr. Guillermo García Segura
Instituto de Astronomía, Universidad Nacional Autónoma de México, Ensenada, Baja California
Galaxies Hidden in the Forest as a new BAO tracer (and other applications)
Galaxies Hidden in the Forest as a new BAO tracer (and other applications)
Dr. Ignasi Pérez Rafols
Universidad Politécnica de Cataluña (UPC), España
Pint of Science 2025 – X Edición
Pint of Science 2025 – X Edición
Espectroscopía 3D: la mejor forma de descifrar la luz de las galaxias
Espectroscopía 3D: la mejor forma de descifrar la luz de las galaxias
Raúl González Díaz
Instituto de Astrofísica de Andalucía (IAA-CSIC)