Mapping the absolute brightness of the sky at low frequencies

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dc.contributor.authorGiovanni De Amici
dc.contributor.authorG. F. Smoot
dc.contributor.authorM. Bensadoun
dc.contributor.authorM. Limon
dc.contributor.authorW. Vinje
dc.contributor.authorC. Witebsky
dc.contributor.authorSergio Torres
dc.contributor.authorAntonio José Mejía Umaña
dc.contributor.authorMiguel Velázquez de la Rosa Becerra
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T16:39:58Z
dc.date.available2026-03-22T16:39:58Z
dc.date.issued1992
dc.descriptionCitaciones: 2
dc.description.abstractUncertainties in the gain and zero‐level of the existing radio and microwave frequency sky surveys often dominate the error budget in studies of anisotropies and spectral distortions of the Cosmic Background Radiation.This paper discusses our existing prototype and the planned instruments and the observation techniques which are necessary for conducting an extended observational campaign to map the total sky brightness. Some experimental difficulties are outlined, and possible solutions are given.
dc.identifier.doi10.1063/1.44014
dc.identifier.urihttps://doi.org/10.1063/1.44014
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/59584
dc.language.isoen
dc.publisherAmerican Institute of Physics
dc.relation.ispartofAIP conference proceedings
dc.sourceLawrence Berkeley National Laboratory
dc.subjectSky
dc.subjectBrightness
dc.subjectCosmic microwave background
dc.subjectSky brightness
dc.subjectRemote sensing
dc.subjectMicrowave
dc.subjectPhysics
dc.subjectComputer science
dc.subjectBrightness temperature
dc.subjectAstronomy
dc.titleMapping the absolute brightness of the sky at low frequencies
dc.typearticle

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