Northern Extended Millimeter Array

Instead of operating one giant telescope, NOEMA relies on several smaller and easily movable antennas placed on tracks. Together, the NOEMA antennas have the resolving power of a telescope with a diameter of more than 1.7 kilometers which is the distance between the outermost antennas.

During observations, the NOEMA antennas function as a single stationary telescope, a technique called interferometry. All NOEMA antennas point towards the same cosmic source. The signals received by each antenna are combined by a supercomputer, a so called correlator, that produces images of outstanding sensitivity and resolution of the astronomical source.

NOEMA functions like a variable lense camera by changing the configuration of its antennas allowing scientists to zoom-in and -out of a cosmic object and obsere the tiniest details. In its most extended configuration NOEMA shows a 0.1 arc second view at 350 GHz revealing the nature of the nearest protostellar disks and the sub-kiloparsec scale of star forming regions of the most distant galaxies. Working with IRAM's second facility, the 30-meter telescope and its wide angle of vision, the result is a giant virtual telescope with a unique set of capabilities.

Compared to optical astronomy, which is sensitive to the hot universe (stars are generally a few thousand degrees Celsius), radiotelescopes that operate in the millimeter wavebands, such as NOEMA, probe the cold universe (around -250 degrees Celsius). NOEMA is able to see the formation of the first galaxies in the universe, to observe super-giant black holes at the center of galaxies, to analyze the chemical evolution and dynamics of nearby galaxies, to detect organic molecules and possible key elements of life and to investigate the formation of stars and the appearance of planetary systems.

The last 30 years, NOEMA has done pioneering work in radio astronomy. It observed the most distant galaxy known to date.[1] Together with the IRAM 30-meter telescope it made the first complete and detailed radio images of nearby galaxies and their gas. NOEMA also obtained the first image of a gas disk surrounding a double star system (Dutrey al. 1994[2]). Its antennas captured for the first time a cavity in one of these disks, a major hint for the existence of a planetary object orbiting the new star and absorbing matter on its trajectory (GG tau, Piétu et al. 2011[3] ). Together, the IRAM facilities have discovered one third of the interstellar molecules known to date (published ApJ, 2018, Brett A. McGuire[4]).

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  The NOEMA observatory
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  The NOEMA observatory, located on the Plateau de Bure in the French Alps
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  The NOEMA antennas looking at the night sky
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  The NOEMA observatory looking at the night sky with the Milky Way.

• List of radio telescopes

• The NOEMA brochure.