Galactic Observations at 31, 42 and 144~GHz with the Mobile Anisotropy Telescope

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dc.creatorPuchalla, J. L.
dc.creatorCaldwell, R.
dc.creatorCruz, K. L.
dc.creatorDevlin, M. J.
dc.creatorDorwart, W. B.
dc.creatorHerbig, T.
dc.creatorMiller, A. D.
dc.creatorNolta, M. R.
dc.creatorPage, L. A.
dc.creatorTorbet, E.
dc.creatorTran, H. T.
dc.date2000-05-22
dc.date.accessioned2026-07-07T01:53:41Z
dc.date.available2026-07-07T01:53:41Z
dc.descriptionWe present multi-frequency maps of a portion of the Galactic Plane centered on a declination of -60 degrees with resolutions ranging from 0.2 to 0.9 degrees. The maps are optimized to detect unresolved source emission and are cross-calibrated against the planet Jupiter. We discuss six millimeter-bright regions, three of which are visible in all bands, and list measured flux densities. Variability is limited to less than 3.8% for all sources seen at 31 and 42 GHz and less than 10% at 144 GHz. Fractional polarization limits smaller than 0.08 are measured for all sources seen at 31 and 42 GHz. No fractional polarization limits are reported at 144 GHz.
dc.description11 pages, 4 postscript figures, Submitted to Astrophysical Journal
dc.identifierhttps://arxiv.org/abs/astro-ph/0005420
dc.identifierhttp://arxiv.org/abs/astro-ph/0005420
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1050
dc.subjectAstrophysics
dc.titleGalactic Observations at 31, 42 and 144~GHz with the Mobile Anisotropy Telescope
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