Welcome to ALMA and the European ALMA Regional Centre!

ALMA (Atacama Large Millimeter/submillimeter Array) is the world's largest ground-based facility for observations in the millimeter/submillimeter regime located on the Chajnantor plateau, 5000 meters altitude in northern Chile. It enables transformational research into the physics of the cold Universe, probes the first stars and galaxies, and directly images the formation of planets. ALMA comprises a giant array of fifty 12-m antennas, which can be configured to achieve baselines up to 16 km. It is equipped with state-of-the-art receivers that cover all the atmospheric windows up to 1 THz. In addition, a compact array of 7-m and 12-m antennas greatly enhance ALMA's ability to image extended sources.

The European ALMA Regional Centre (ARC) provides the interface between the ALMA project and the European science community. It supports its users mainly in the areas of proposal preparation, observation preparation, data reduction, and data analysis.

Below you can read the latest Announcements from the European ARC Network.. More details and up-to-date information can be found in the News section and the ALMA Science Portal.

Celebrating ALMA Band 2 Production Completion

Published: 24 Jun 2026

On 16 June 2026, EASC hosted the ALMA Band 2 Production Completion Event. 36 participants from the Band 2 consortium, contributing European institutes, industry partners, and the National Astronomical Observatory of Japan (NAOJ) travelled to ESO Garching to celebrate this important milestone for ALMA. Together with ESO staff, more than 70 people attended the associated workshop and celebration activities throughout the day.

ALMA User Survey on Advanced Data Products

Published: 24 Jun 2026

Advanced data products (ADPs) are becoming increasingly important at modern radio observatories, helping transform complex observational datasets into more accessible, science-ready resources. Products such as enhanced images, spectral products, catalogs, or other higher-level derived datasets can reduce the effort required for scientific analysis and broaden access to archival data. To better understand how such products are currently used, and what additional capabilities may be most valuable to the community in the future, the Advanced Data Products Coordination Group (ADPCG), with members from various radio observatories and the broader community, is conducting a short survey on the usage and potential needs for advanced data products. We warmly encourage all members of the community to participate and share their perspective.

ADPCG Community Survey 2026 – Fill out form

Cycle 13 Proposal Submission Statistics

Published: 12 Jun 2026

A detailed report of the Cycle 13 Proposal Submission Statistics is now available. The report provides a summary of items such as the number of submitted proposals and time requested, subscription rates, and comparisons with the number of hours requested in previous Cycles.

In Cycle 13, the number of proposals and requested time reached all-time highs. The European oversubscription rate also reached an all-time high of 10.2.

The report can be downloaded as a pdf document.

Upcoming Release of Observatory Project Data for "An ALMA Band 1 Survey of the Hubble Deep Field South"

Published: 11 Jun 2026

The ALMA Observatory is starting the release process of the data acquired in one of the Observatory Projects, 2024.A.00047.S. The status of the data delivery can be checked through this link. The same link can be used to download the data once it is delivered. ALMA Science Archive links for all the Observatory Projects can also be accessed from this main page for the Observatory Projects.

 

Kick-off for a new study on SIS development for Band 9

Published: 19 May 2026

In preparation for the Wideband Sensitivity Upgrade (WSU) programme, a team lead by Faouzi Boussaha from the Instrumental Research and Development group at LUX – Paris Observatory (France) has started a new ALMA development study to contribute to the development of the next generation of SIS (Superconductor–Insulator–Superconductor) detectors for ALMA's Band 9. The goal of the study is to double the instantaneous IF bandwidth and significantly increase the sensitivity, requiring a new generation of ultra-sensitive detector elements known as SIS junctions. Specifically, the study plans to use the Aluminium Oxide technology but will investigate new substrates such as silicon on insulator.

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