Results from the First Flight of BAM

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dc.creatorTucker, G. S.
dc.creatorGush, H. P.
dc.creatorHalpern, M.
dc.creatorTowlson, W.
dc.date1996-09-17
dc.date.accessioned2026-07-07T02:21:55Z
dc.date.available2026-07-07T02:21:55Z
dc.descriptionA new instrument, BAM (Balloon-borne Anisotropy Measurement), designed to measure cosmic microwave background (CMB) anisotropy at medium angular scales was flown for the first time in July of 1995. BAM is unique in that it uses a cryogenic differential Fourier transform spectrometer coupled to a lightweight off-axis telescope. The very successful first flight of BAM demonstrates the potential of the instrument for obtaining high quality CMB anisotropy data.
dc.description6 pages, 3 EPS figures, TeX. To appear in Proceedings of the XXXIst Moriond Meeting "Microwave Background Anisotropies", Les Arcs (France), March 16-23 1996
dc.identifierhttps://arxiv.org/abs/astro-ph/9609108
dc.identifierhttp://arxiv.org/abs/astro-ph/9609108
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10683
dc.subjectAstrophysics
dc.titleResults from the First Flight of BAM
dc.typetext

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