The ALMA Back-End
BAUDRY, Alain
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
See more >
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
BAUDRY, Alain
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
< Reduce
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Language
en
Autre document
This item was published in
2006
English Abstract
The Atacama Large Millimeter Array is designed to produce excellent im- ages in spectral lines and continuum, to detect distant galaxies like our Milky Way and to image proto-stellar discs in the nearest molecular clouds. ...Read more >
The Atacama Large Millimeter Array is designed to produce excellent im- ages 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 ac-complish these goals, signals from the ALMA antennas must be processed and transmitted to the technical build-ing 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 Euro-pean Institutes under ESO coordination.Read less <
Origin
Hal imported