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.

Development study on ALMA uv coverage assessment completed

Published: 28 Aug 2024


A new development study has introduced new methods to define and measure the maximum recoverable angular scale in ALMA observations. These methods will improve imaging quality and allow for better predictions for observation scheduling.

Contributed by Dirk Petry.

Video on ALMA's Wideband Sensitivity Upgrade released

Published: 28 Aug 2024

In June 2024, the ESO workshop "The Promises and Challenges of the ALMA Wideband Sensitivity Upgrade" was held in Garching to introduce all details of this ambitious upgrade project to the user community (see the announcement in July's newsletter). Following this and in an effort to further advertise this upgrade to the community and the public in general, ESO has just released the video "ALMA's extreme makeover: the Wideband Sensitivity Upgrade". You can watch the video here.

Contributed by Maria Diaz Trigo.

First Joint VLT/ALMA Observing Proposal successfully completed

Published: 12 Aug 2024

From Cycle 10, it has been possible to propose for joint VLT and ALMA observations. The first joint VLT/ALMA observing proposal has now been completed (prog ID 113.269Z, PI Benisty). Multi-epoch observations of a protoplanetary disc using VLT/SPHERE and ALMA revealed the suface and midplane layers of the disc. These observations aim to understand the mechanisms and timescale of cooling, which are critical to understanding disc evolution.

Completion of the study on AlN SIS junctions technology development

Published: 26 Jul 2024

A study by the Group for Advanced Receiver Development (GARD, Sweden) to develop new fabrication technology for sub-micron size Aluminium Nitride (AlN) barrier Superconductor Insulator Superconductor (SIS) junctions has been successfully completed. These SIS junctions are at the core of most ALMA receivers where the sky signal is mixed with the Local Oscillator to tune the receivers to the desired frequency. 

Completion of the ALMA development study on the Atmospheric Model

Published: 26 Jul 2024

A development study aimed to validate and improve the current atmospheric radiative transfer model implemented for ALMA (atmospheric transmission model, ATM) has been successfully completed. The model is important for both planning and helping in the calibration of ground-based observations at millimeter and submillimeter wavelengths.

Quick Links