Actualidad
Eventos
Agenda
High energy blazar physics in the Multi-Messenger context
High energy blazar physics in the Multi-Messenger context
Yuri Kovalev
Max Planck Institute for Radio Astronomy
SO Colloquium – SDSS-V and beyond: status of the LVM and the new AS5 proposal
SO Colloquium – SDSS-V and beyond: status of the LVM and the new AS5 proposal
Sebastián Sánchez
Instituto de Astronomía, UNAM
HAYDN: A Next-Generation ESA Mission Concept for Stellar Structure and Evolution and its impact on exoplanet and galaxy formation
HAYDN: A Next-Generation ESA Mission Concept for Stellar Structure and Evolution and its impact on exoplanet and galaxy formation
Andrés Moya Bedón
Universitat de València
SO Colloquium – The formation of high-altitude clouds on terrestrial planets
SO Colloquium – The formation of high-altitude clouds on terrestrial planets
Anni Määttänen
LATMOS laboratory, Centre national de la recherche scientifique (CNRS)
Archivo
From cluster detection to galaxy alignment: an overview of SCALE with S-PLUS survey
From cluster detection to galaxy alignment: an overview of SCALE with S-PLUS survey
Lia Doubrawa
University of Helsinki - Finland, Universidade de São Paulo - Brazil
Darwin y las galaxias
Darwin y las galaxias
Emilio J. Alfaro
Instituto de Astrofísica de Andalucía (IAA-CSIC)
KM3-230213A: the ultra-high-energy neutrino detected in KM3NeT
KM3-230213A: the ultra-high-energy neutrino detected in KM3NeT
Sergio Navas Concha
University of Granada
Simulations to unlock Micro-Arcsecond Astronomy with La Palma Quantum Interferometry (LPQI)
Simulations to unlock Micro-Arcsecond Astronomy with La Palma Quantum Interferometry (LPQI)
Nitu Rai
Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital
SO Colloquium: MOSAIC: the multi-object spectrograph for the ELT
SO Colloquium: MOSAIC: the multi-object spectrograph for the ELT
Roser Pelló
Laboratoire d'astrophysique de Marseille (LAM)
SO Colloquium: Planetesimal vs. Pebble Accretion
SO Colloquium: Planetesimal vs. Pebble Accretion
Steve Desch
Arizona State University, USA
SO Colloquium: The Earth 2.0 (ET) Space Mission
SO Colloquium: The Earth 2.0 (ET) Space Mission
Jian Ge
Shanghai Astronomical Observatory
MeerKAT imaging of nearby galaxies
MeerKAT imaging of nearby galaxies
Juliana Saponara
Instituto Argentino de Radioastronomia (IAR)
Mirar los cielos: el misterio de la Luna
Mirar los cielos: el misterio de la Luna
Monserrat Villar Martín
Centro de Astrobiología (INTA-CSIC)
First Glimpses of the Extragalactic Gamma-ray Sky with LST-1: Paving the Way to CTAO
First Glimpses of the Extragalactic Gamma-ray Sky with LST-1: Paving the Way to CTAO
Jorge Otero-Santos
INFN Sezione di Padova
SO Colloquium: The future science of CTAO
SO Colloquium: The future science of CTAO
Giacomo Bonnoli
INAF - Istituto Nazionale di Astrofisica, Osservatorio Astronomico di Brera - Sede di Merate
SO Colloquium: Pre-CTAO Science with LST: Current and Expected Results
SO Colloquium: Pre-CTAO Science with LST: Current and Expected Results
Prof. Pol Bordas
IEEC - ICC - Universitat de Barcelona
SO Colloquium: Galactic Centres and their high-energy multimessenger Phenomena
SO Colloquium: Galactic Centres and their high-energy multimessenger Phenomena
Elena Rossi
University of Leiden, The Netherlands
A SITELLE overview of interacting galaxies and supernova remnants
A SITELLE overview of interacting galaxies and supernova remnants
Prof. Laurent Drissen
Université Laval, Québec
Extreme gamma-ray pulsars (and what CTAO can say about them)
Extreme gamma-ray pulsars (and what CTAO can say about them)
Giovanni Ceribella
Max Planck for Physics (MPP)
The role of groups in galaxy evolution: the importance of the pre-processing effect
The role of groups in galaxy evolution: the importance of the pre-processing effect
Paulo Afranio Lopes
Observatorio do Valongo, Rio de Janeiro, Brasil
