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The ALMA Back-End

hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorBAUDRY, Alain
dc.contributor.authorBIANCAT MARCHET, Fabio
dc.contributor.authorKURLANDCYK, Hervé
dc.contributor.authorROSSI, Silvio
dc.date.issued2006
dc.descriptionThe Messenger vol 125 (2006), p. 37-40 (2006)
dc.description.abstractEnThe 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.
dc.language.isoen
dc.title.enThe ALMA Back-End
dc.typeAutre document
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]
hal.identifierhal-00130898
hal.version1
hal.audienceNon spécifiée
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00130898v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2006&rft.au=BAUDRY,%20Alain&BIANCAT%20MARCHET,%20Fabio&KURLANDCYK,%20Herv%C3%A9&ROSSI,%20Silvio&rft.genre=unknown


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