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.

Cycle 13 Call for Proposals now open

Published: 19 Mar 2026

Cycle 13 Call for Proposals has been released. Cycle 13 introduces two new developments: Band 2 (67–116 GHz) will be offered for all of ALMA, and the new web-based Observing Tool (OT) will replace the desktop version. This cycle will offer long baseline configurations (C9 and C10). Further details of the capabilities offered can be found in the Proposer's Guide.

We particularly encourage proposals using long baselines at lower frequencies (Bands 1-4), high-frequency observations (Bands 8-10) and stand-alone ACA. 

As always, users are strongly encouraged to submit their proposals early, especially in view of the introduction of the new web-based OT. The Emergency Helpdesk will be open for the 3 days leading up to the proposal deadline. 

 

Cycle 13 proposal preparations events across Europe

Published: 18 Mar 2026

The European ALMA Regional Centre (ARC) network is organising virtual and in-person proposal preparation events related to the Cycle 13 Call for Proposals across Europe.  

An overview of the activities and information about participating can be found here

Introducing the new web-based ALMA Observing Tool (OT)

Published: 18 Mar 2026

ALMA is pleased to announce that a web-based interface of the ALMA Observing Tool (OT) will replace the previously used desktop-based OT for the Cycle 13 Call for Proposals. The web-based OT offers the same functionality as the desktop-based OT. The new interface offers a modernized and optimized view while retaining the same familiar workflow and structure. Proposal drafts will now be automatically saved within the system, without the need to save local files. 

Streaming Visibility Processing for ALMA

Published: 16 Mar 2026

In a recently concluded development study, a small team at ASTRON, The Netherlands Institute for Radio Astronomy, investigated the concept of Streaming Visibility Processing (SVP) for ALMA. The key idea behind the SVP concept is to stream the visibilities produced by the ALMA correlator into the (initial) data processing stages without storing them first. SVP performs initial visibility processing in real-time up to the point where the data is reduced to more tractable rates without detrimental effects on the scientific quality of the end products. Further details are in the final report of the streaming visibility processing study and by following the 'read more' link.

Band 2 will be offered in Cycle 13 for ALMA 12m array

Published: 02 Feb 2026

Band 2 (67-116 GHz) is anticipated to be offered on the 12m Array from the start of Cycle 13 (October 2026). As with previous new band introductions (e.g. Band 1), the exact start date and number of available antennas may be subject to operational and technical constraints. Based on current receiver integration progress, up to 43 Band 2 receivers may be available at the start of the cycle.

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