Towards ALMA2040: An update from the European community and invitation to contribute
Stefano Facchini (U. Milan), Jacqueline Hodge (Leiden U.), Jes J{\o}rgensen (U. Copenhagen), Eva Schinnerer (MPIA), Gie Han Tan (TU Eindhoven), Tom Bakx (Chalmers), Andrey Baryshev (U. Groningen), Maite Beltran (INAF Firenze), Leindert Boogaard (Leiden U.)

TL;DR
This paper discusses the future of millimeter/submillimeter astronomy with ALMA by 2040, emphasizing community-driven planning for a next-generation facility amid evolving observational capabilities.
Contribution
It introduces the ALMA2040 initiative, outlining a community-driven effort to define scientific goals and technical visions for a transformative future (sub-)mm observatory.
Findings
Summarizes the current status of ALMA2040 planning.
Synthesizes outcomes from 2025 workshops.
Outlines next steps for a reference design.
Abstract
Over the last 15 years, the Atacama Large Millimeter/submillimeter Array (ALMA) has revolutionized astrophysics by providing unprecedented resolution and sensitivity in observing the cold universe, including the formation of stars, planets, and galaxies. With groundbreaking discoveries ranging from the first detailed images of protoplanetary disks to the kinematics of galaxies in the Epoch of Reionization, ALMA has showcased the vast discovery potential of the (sub-)mm wavelength regime. However, in another 15 years from now--in the 2040s--the science landscape will have changed dramatically as new major observational facilities will have started their operations or have come towards advanced maturity in their scientific outcome (e.g., JWST, Rubin Observatory, ELT, Euclid, Gaia, Plato, Ariel, Roman Space Telescope, SPHEREx, LiteBIRD, LISA, SKA and others). At the same time, ALMA's…
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Taxonomy
TopicsSuperconducting and THz Device Technology · Radio Astronomy Observations and Technology · Astronomy and Astrophysical Research
