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EAS 2026
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Special Session SS13
AGN populations in large sky radio surveys
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S1: Cosmology with wide spectroscopy surveys
S2: Science with gravitational lensing in the multi-space …
S3: The stellar route to H0: not only Classical Cepheids
S4: Preparing for multi-messenger observations with LISA and PTAs
S5: Diverse Eyes, shared vision: Euclid, LSST, SKA, Roman and …
S6: Shaping galaxies and their gaseous environment in the early …
S7: Gaia, at the dawn of Gaia DR4, preparing for DR5 and beyond
S8: A multi-faceted view of accretion at super-Eddington rates
S9: The Rise and Shine of Rapidly Assembling Galaxies and Black …
S10: Euclid: the first 2000 square degrees of the cosmos
S11: Globular clusters as tracers of galaxy formation and …
S12: Supernovae and their remnants: from stellar death to …
S13: Massive supergiants in focus: single, binary and stellar …
S14: From small-scale solar phenomena to stellar contexts: …
S15: AI for astronomical discovery: Foundation Models, Machine …
S16: Future of European Astronomy
SS1: Unlocking the secrets of dark matter with low surface …
SS2: Ultra-faint dwarf galaxies: the final frontier?
SS3: Out of the box, moving from morpho-kinematic classes to …
SS4: The interplay between gravity and baryons: insights from low …
SS5: UV-bright star-forming clumps as tracers of galaxy …
SS6: From molecular clouds to galaxy clusters: towards a unified …
SS7: Mind the gap: Bridging resolved and unresolved young stellar …
SS8: Local group star formation in the conditions of cosmic noon: …
SS9: Multi-phase molecular gas in nearby and distant galaxies …
SS10: Resolving the missing details for the Milky Ways accretion …
SS11: Young stellar structures in the Milky Way
SS12: Accretion disk winds across mass scales
SS13: AGN populations in large sky radio surveys
SS14: From shadows to Jets: BH science with the EHT
SS15: Neutrinos from the Dark: unveiling hadronic processes in …
SS16: Precision measurements of astrophysical jets across scales …
SS19: Timing of the accretion flow in compact objects: X-ray …
SS18: TeV astronomy: setting up the new generation of Cherenkov …
SS19: ARRAKIHS: a space mission dedicated to low surface …
SS20: SKAO science verification and beyond: preparing users for …
SS21: Preparing for PLATOs science data: mission insights and …
SS22: Getting ready for Science with the Nancy Grace Roman Space …
SS23: Transformative science from 30-Meter Class telescopes in the …
SS24: WST in the 2040s landscape: the power of synergies.
SS25: Optical Interferometry in the next decade: Science, …
SS26: Planning the future of large-scale (sub-)mm astrophysics
SS27: The Vera Rubin Observatory Legacy Survey of Space and Time: …
SS28: WEAVE and 4MOST: whole-sky spectroscopic coverage through …
SS29: The dance of stars within galaxies: transients, their …
SS30: A synoptic view of star formation with the VLTI and JWST
SS31: Exotic populations in star clusters seen through the lens of …
SS32: Kilonovae: further insights from theory and observations
SS33: Pushing the frontiers: precision spectroscopy of FGK stars
SS34: EST, the next-generation solar telescope
SS35: Exoplanets and the Galactic environment
SS36: Synergies between JWST and the ELT for the study of star and …
SS37: Planet formation in sub-structured disks: from dust traps to …
SS38: Machine Learning for Spectroscopy: unlocking galaxy and AGN …
SS39: Early Career astronomers and their supporters
SS40: Next steps towards greener astronomy
SS41: European forum of astronomical communities
SS42: Challenges ahead: how to deal with interference from …
SS43: Saving astronomy in Ukraine: what can we do as a community?
SS44: The changing face of astronomy publishing
LS1: Getting the most out of ESO data: a hands-on session on the …
LS2: The ESA science program
LS3: Astronomy on Tap Europe Networking Lunch
LS4: The ESA Space Science Archives
LS5: Evaluating IDEAs (Inclusion, Diversity, Equity and …
LS6: EPFL Space Associations
LS7: VLTI 2026: entering the new sensitivity era
European Astronomical Society