Galactic Observations at 31, 42 and 144~GHz with the Mobile Anisotropy Telescope
J. L. Puchalla, R. Caldwell, K. L. Cruz, M. J. Devlin, W. B. Dorwart, T. Herbig, A. D. Miller, M. R. Nolta, L. A. Page, E. Torbet, H. T. Tran
Abstract
We 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.
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