arXiv · 0812.2450
GMIMS: The Global Magneto-Ionic Medium Survey
Abstract
The Global Magneto-Ionic Medium Survey (GMIMS) is a project to map the diffuse polarized emission over the entire sky, Northern and Southern hemispheres, from 300 MHz to 1.8 GHz. With an angular resolution of 30 - 60 arcmin and a frequency resolution of 1 MHz or better, GMIMS will provide the first spectro-polarimetric data set of the large-scale polarized emission over the entire sky, observed with single-dish telescopes. GMIMS will provide an invaluable resource for studies of the magneto-ionic medium of the Galaxy in the local disk, halo, and its transition.
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M. Wolleben, T. L. Landecker, E. Carretti, J. M. Dickey, A. Fletcher, B. M. Gaensler, J. L. Han, M. Haverkorn, J. P. Leahy, N. M. McClure-Griffiths, D. McConnell, W. Reich, A. R. Taylor. 2008-12-12. GMIMS: The Global Magneto-Ionic Medium Survey. https://doi.org/10.1017/s1743921309030117
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