The ALMA Back-End

Details The ALMA Back-End The ALMA Back-End

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006msngr.125...37b&link_type=abstract

The Messenger, volume 125, page 37

Computer Science

Scientific paper

The Atacama Large Millimeter Array is designed to produce excellent images in spectral lines and continuum, to detect distant galaxies like our Milky Way and to image proto-stellar discs in the nearest molecular clouds. To accomplish these goals, signals from the ALMA antennas must be processed and transmitted to the technical building in a format ready to be accepted by the correlator. The ALMA Back-End provides this in a loss-free, reliable and flexible way. In the following an overview is given of the ALMA Back-End subsystems developed in various European Institutes under ESO coordination.

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