The Very Small Array - status report

Simple item page
dc.creatorJones, Michael E.
dc.creatorScott, P. F.
dc.date1998-04-17
dc.date.accessioned2026-07-07T02:26:37Z
dc.date.available2026-07-07T02:26:37Z
dc.descriptionWe are contructing an interferometric telescope, the Very Small Array, to study the cosmic microwave background on angular scales 0.2--4.5 degrees. The physical layout and electronic design of the telescope are optimised to give maximum protection from systematic effects, while still providing sufficient sensitivity to make high signal-to-noise images. A prototype single baseline is currently being tested, with scientific results expected during 2000.
dc.description4 pages, 3 figures. To be published in proceedings of the 33rd Rencontres de Moriond, Fundamental Parameters in Cosmology
dc.identifierhttps://arxiv.org/abs/astro-ph/9804175
dc.identifierhttp://arxiv.org/abs/astro-ph/9804175
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12348
dc.subjectAstrophysics
dc.titleThe Very Small Array - status report
dc.typetext

Files

Collections

arXiv